This galaxy presents a generally smooth, elliptical morphology. The light distribution is concentrated towards the center, with a gradual decrease in intensity moving outward, exhibiting a radial profile. It exhibits a slight elongation rather than a perfectly circular appearance. The galaxy's color profile suggests an older stellar population, with a subtle reddish tint. There are slight indications of minor disturbances, such as a slight asymmetry in the outer regions of the galaxy, but no clear signs of a major merger event or strong tidal interactions. The central region appears bright and dense, suggestive of a significant concentration of stars. There is a lack of discernible spiral arm structure or prominent dust lanes.
