The galaxy presents a largely smooth morphology, indicative of a relatively evolved system. The light distribution is concentrated towards the center, with a bright, nearly spherical central bulge exhibiting a yellowish-white hue, potentially suggesting a population of older stars. This central region appears relatively quiescent. Extending outward from the bulge is a faint, diffuse disk component. Subtle color gradients are present, with a slight bluish tint observed in the outer regions, suggestive of some ongoing, albeit low-level, star formation. No prominent spiral arm structures are apparent, and there are no obvious signs of active galactic nuclei activity or major mergers, though there appears to be a very minor distortion in the shape of the outer halo on one side of the galaxy. The overall impression is that of a galaxy with a significant spheroidal component and limited ongoing star formation.
