The galaxy appears to be a relatively smooth, elliptical or lenticular system. It exhibits a concentrated central bulge which transitions gradually into a fainter, diffuse halo. The overall shape is somewhat rounded, with only a slight elongation. There is no obvious dust lane or spiral structure, which is consistent with an older stellar population and a low rate of star formation. The galaxy's color is predominately yellowish, suggesting a population of older, redder stars. There is no indication of ongoing merger activity or significant tidal disturbances. The galaxy is moderately sized.
