This galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a concentrated central bulge. The light profile suggests a centrally-concentrated stellar population with a lack of significant spiral arm structure. It is generally round in shape, without any signs of major distortions or tidal features indicative of recent major merger activity, though very slight disturbances cannot be ruled out. The color index, judging by the yellow/gold hue, indicates a population of older stars with low star formation, which would indicate a low specific star formation rate. The overall apparent size is small, suggesting it is at a considerable distance. 