The galaxy exhibits a generally smooth morphology, with a slightly elongated profile. The light distribution indicates a concentrated central region, potentially a bulge, surrounded by a more diffuse, extended halo. The overall color appears relatively red, suggestive of an older stellar population with suppressed star formation. There is a subtle indication of a possible disk structure, although the smoothness of the light distribution predominates. No signs of major mergers or significant tidal disturbances are apparent. The galaxy presents as a transition type, leaning towards an early-type system based on its smoothness, concentration, and redder color.
