The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge with a diffuse halo extending outwards. The light profile appears relatively uniform, lacking distinct spiral arms or prominent dust lanes. The galaxy's color index suggests the presence of an older stellar population, as indicated by the redder hue, although there is evidence of ongoing star formation, especially toward the central area. The galaxy appears slightly elongated, deviating marginally from a perfect circular shape. The overall appearance is consistent with a relatively quiescent system, possibly an early-type galaxy undergoing a period of slow star formation. There is no obvious visual evidence of any major merging activity or significant tidal disturbances.
