The galaxy appears to be elliptical in shape, with a smooth, diffuse light distribution, and a bright, concentrated central bulge. The lack of defined spiral arms or significant dust lanes suggests a relatively old stellar population. The galaxy exhibits a dominant yellow-white hue, indicative of older stars with lower rates of star formation, though bluer colors are visible in the outer regions. The overall morphology is consistent with an early-type galaxy that is relatively undisturbed. There are no visual indications of ongoing major mergers or tidal interactions.
