The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a centrally concentrated light distribution, with a bright core region that gradually fades into the outer regions. There's little evidence of prominent spiral arms or distinct disk features. The overall color appears somewhat blueish-white, suggesting a population of young to intermediate-age stars. There's a slight elongation, but the galaxy is mostly round. Based on the lack of obvious distortions, it appears to be relatively undisturbed, with no major signs of ongoing mergers or tidal interactions. There is a slight hint of some low-level disturbances or faint extensions in the halo.
