The galaxy presents as a centrally concentrated, somewhat elliptical object. Its color appears predominantly greenish, suggesting prominent emission lines at those wavelengths. The light distribution is fairly smooth, with a gradual fall-off in brightness from the center to the edges. There is little evidence of spiral arm structure or prominent dust lanes; however, some minor distortions or subtle disturbances are present. The overall morphology implies an evolved system with a relatively homogenous stellar population, though the presence of a faint disk or a small merging event can't be ruled out.
