The galaxy presents as a centrally concentrated object, appearing largely smooth in morphology. It exhibits a bright, diffuse core which gradually fades into the surrounding halo. There is very little discernible structure, such as spiral arms or dust lanes. The overall shape appears to be somewhat elliptical, though it tends towards roundness. There is no obvious indication of major mergers or significant tidal disturbances in the immediate vicinity. The galaxy displays a yellowish hue, which suggests a stellar population dominated by older stars. The color also indicates that the galaxy is likely undergoing only a low level of star formation.
