The galaxy presents as a relatively smooth, centrally concentrated elliptical or lenticular system. Its overall color suggests a moderate population of older stars, possibly with a faint disk component. There is a slight elongation in the morphology, deviating marginally from a perfectly circular shape. A central bulge region appears bright and somewhat redder in comparison to the outer regions. The outer regions exhibit a fainter, bluer hue, which might indicate pockets of younger stellar populations. The galaxy shows no obvious signs of major mergers or strong tidal disturbances, although there may be minor asymmetry. The galaxy's light profile appears to fade gradually towards the edges.
