This galaxy presents a generally smooth, elliptical morphology, although some finer structures are visible upon closer inspection. The central region exhibits a higher surface brightness, appearing nearly spheroidal, with a concentration of light suggesting a substantial bulge component. The overall color is slightly bluer in the core, transitioning to redder hues in the outer regions, which could indicate differing stellar populations or dust content across the galaxy.

There are hints of faint, extended features or tidal tails, suggesting possible interactions or past merger events. The light distribution appears relatively uniform without strong spiral arm structures. Disturbances in the main body of the galaxy are visible. There is some evidence of asymmetry. The galaxy is moderately luminous, but does not appear to be undergoing vigorous star formation.
