The galaxy presents as a moderately luminous object, appearing somewhat flattened or elliptical in shape. A central bulge dominates the galaxy's morphology, exhibiting a yellowish-orange hue suggestive of an older stellar population. Surrounding the central bulge is a fainter, more diffuse disk or halo, which displays a slightly bluer tint. This suggests the presence of a younger stellar population, possibly regions of ongoing star formation. There is a suggestion of some degree of disturbance or interaction. The galaxy does not exhibit any strong spiral arm structure or other prominent features, making it difficult to classify with certainty. It appears relatively isolated, with no obvious signs of a major merger event in progress, however there may be a faint tidal stream on one edge.
