The galaxy appears as a fairly smooth elliptical, exhibiting a concentrated central bulge that fades into a more diffuse halo. The galaxy's color profile suggests an older stellar population, with a redder hue prominent throughout. There is little evidence of ongoing star formation, as indicated by the lack of blue light or distinct HII regions. The overall morphology points to a galaxy that has largely exhausted its gas supply, leading to a cessation of significant star birth. It appears spheroidal. The object is isolated and shows no strong signs of tidal disturbances or interactions with neighboring galaxies. No dust lanes or prominent spiral arm structures are visible. The elliptical shape is almost completely round.
