The galaxy presents an overall smooth morphology, exhibiting a concentrated central bulge that appears near-spherical. The color profile suggests a population of older stars, especially within the central region, showing a shift towards redder wavelengths. The galaxy has a moderate ellipticity, deviating slightly from a perfectly circular shape. There is no clear evidence of spiral arm structure or a distinct disk component. Subtle disturbances are noticeable, potentially indicating minor gravitational interactions or internal dynamic processes. There is a possible secondary, smaller component nearby, but determining if this is a true satellite galaxy or a projection effect requires further investigation. The galaxy shows an overall smooth profile, with no apparent strong tidal features, jets, or active galactic nucleus signatures. The gradual radial decrease in surface brightness suggests a relatively relaxed system.
