The galaxy presents as a relatively smooth, rounded structure. The central region exhibits a concentrated, bright yellowish hue, suggestive of a substantial population of older stars. There is a gradual decrease in luminosity from the center outwards. The faint, diffuse outer regions lack any clearly discernible spiral arms or disk features. The overall morphology indicates an elliptical galaxy, possibly an early-type spiral with a dominant bulge and weak disk component. There is no clear evidence of recent or ongoing major mergers or significant tidal disturbances.
