This galaxy exhibits a relatively smooth, elliptical morphology with a concentrated central bulge. The light distribution appears predominantly uniform, lacking prominent spiral arms or distinct dust lanes. Color gradients suggest an older stellar population, with the central region displaying a yellowish hue indicative of evolved stars. A faint, diffuse halo surrounds the core, gradually fading into the background sky. There is no indication of ongoing major mergers or significant tidal disturbances in the immediate vicinity of this system. The galaxy's overall appearance suggests a relaxed, evolved system that is likely quiescent in terms of star formation activity.
