The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The color profile transitions from a yellowish core to a bluer halo, suggesting a mix of stellar populations. The central region, likely composed of older stars, exhibits a more redshifted color. The outer regions are indicative of a population of younger, bluer stars. There is some minor irregularity in the shape, possibly indicative of an interaction or minor disturbance, but the overall morphology appears largely undisturbed. The galaxy is moderately compact, showing a relatively high surface brightness. No spiral arms or distinct disk-like features are discernible.
