The galaxy presents a largely smooth, elliptical morphology. There is a concentrated central bulge region that transitions gradually outward into a more diffuse halo. The light distribution exhibits a radially decreasing profile, with the core being significantly brighter than the outer regions. Color gradients are subtle, but there appears to be a slight bluer hue towards the outskirts of the galaxy, suggesting some ongoing star formation activity in these regions, relative to the core, where star formation has likely ceased. There is no evidence of spiral arms, bars, or significant dust lanes. The overall structure suggests a system that has undergone significant dynamical relaxation. The observed shape is consistent with a nearly spherical or slightly flattened ellipsoid. There does not appear to be any significant tidal disturbance or signs of recent merger activity.
