The galaxy presents as a moderately luminous, elongated system with a smooth appearance. Its structure is dominated by a central bulge region that appears relatively featureless. The galaxy exhibits a redder color profile, suggesting a population of older stars and a reduced rate of current star formation. There is a subtle indication of a faint disk component, but it is poorly defined. There is no clear evidence of ongoing mergers or major tidal disturbances affecting its morphology. The overall morphology appears to be consistent with an elliptical galaxy, likely with a substantial stellar mass.
