The galaxy presents a somewhat elliptical morphology, appearing relatively smooth in structure. The central region exhibits a higher surface brightness, suggesting a concentration of older stars in the bulge. Moving outward from the center, the light appears to gradually fade, with what seems to be a disk component implied, though it lacks distinct spiral arms. The overall color appears to be leaning towards redder hues, suggesting an older stellar population. There is no obvious indication of a major ongoing merger event or significant tidal disruptions, but the slight asymmetry could potentially suggest a minor interaction in the recent past. The galaxy seems fairly quiescent in terms of active star formation.
