The galaxy presents a complex morphology, exhibiting characteristics of both a disk galaxy and potentially undergoing a minor interaction. It appears as a somewhat disrupted spiral galaxy. The disk component is not clearly defined but inferred from a slight elongation and non-uniform surface brightness distribution.

The central bulge region presents a smooth, concentrated light profile, transitioning outwards into a more diffuse, less structured disk. There are indications of disturbed features, possibly tidal arms or debris, emanating from the galaxy. The galaxy exhibits a slight asymmetry, potentially suggestive of a minor merger or tidal interaction. The color of the central bulge appears redder, indicative of an older stellar population, while the outer regions show bluer tints, consistent with ongoing star formation. Overall star formation appears to be low to moderate.

The size of the galaxy is moderate, occupying a substantial angular extent in the image. Evidence of dust lanes within the disk is subtle but possibly present, contributing to the complex morphology. The galaxy is likely at a considerable distance, indicated by its small angular size and the presence of significant redshift.
