The galaxy presents as an elliptical morphology, with a concentrated central bulge and a fainter, diffuse halo extending outwards. The galaxy exhibits a yellowish hue, which suggests a population of older stars. The smooth light distribution reinforces the notion of a relatively quiescent stellar population. It has no discernible spiral arms or dust lanes. There may be a tidal tail visible on one side of the galaxy, this would indicate a prior or ongoing merger.