The galaxy presents a largely smooth and elliptical morphology. Its color profile indicates a higher concentration of older stellar populations, particularly within the central bulge. The light is dominated by yellow hues, suggesting a paucity of ongoing star formation. There is no evidence of a prominent or well-defined disk component. The galaxy shows a generally round profile, with no apparent tidal features, major disturbances, or indication of active merging events. The morphology suggests the galaxy is an evolved system.