The galaxy presents a largely elliptical morphology. A central bulge is prominent, exhibiting a bright, concentrated luminosity. The color gradient suggests an older stellar population concentrated within the core, trending towards redder wavelengths. Fainter, diffuse emission extends outwards from the central region, lacking any distinct spiral arm structure or prominent dust lanes. The overall smoothness of the light distribution indicates that the system has undergone significant dynamical relaxation. There is faint evidence of some minor asymmetry in the outer isophotes, possibly suggestive of a past minor merger or tidal interaction. Star formation appears to be subdued throughout the galaxy, with little to no evidence of young, blue stars or HII regions. The halo appears to be relatively devoid of bright stellar clusters or globular clusters, with the galaxy generally exhibiting a uniform, featureless appearance.
