The galaxy presents as a slightly elongated, disk-shaped structure. The central bulge appears bright and concentrated, with a yellowish-white hue. This coloration suggests a population of older stars dominating the core. Surrounding the bulge, a fainter, bluer disk is visible. The blue color suggests the presence of younger, hotter stars and ongoing star formation within the disk. The disk appears relatively smooth, lacking prominent spiral arm structures, indicating that it is likely a lenticular galaxy. The outer edges of the disk fade gradually into the background, showing a relatively high degree of symmetry. There are some hints of minor disturbances or asymmetries in the outer regions. Overall, it is a relatively smooth, well-defined galaxy with a clear bulge and disk structure.
