The galaxy presents as a spiral type, exhibiting a disk-like structure with a slightly elongated form. The morphology is dominated by a bulge, which displays a smooth and concentrated light distribution, transitioning gradually into the surrounding disk. The arm structure is not particularly well-defined, appearing somewhat flocculent. The light distribution suggests a lack of strong, ongoing star formation within the arms. The color gradient indicates a population of older stars overall, with some regions of bluer emission, especially towards the outer parts of the disk. The galaxy has a disturbed morphology with what appears to be some minor disturbances present.
