The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge, and a fainter, more diffuse halo. Color analysis indicates a significant population of older stars, with a dominant yellow-red hue throughout the galaxy's structure. There is little evidence of recent or ongoing star formation within the visible spectrum. The overall form appears somewhat disturbed, possibly indicating a minor interaction or past merger event. Its shape is largely in between round and elliptical with most likely no merging currently happening, but small disturbances could be taking place.