The galaxy presents as a relatively smooth, elliptical-like structure. The light distribution exhibits a centrally concentrated bulge region with a fairly rapid decline in luminosity as one moves outwards. There are no distinct spiral arm features visible. The overall color is indicative of a galaxy population dominated by older stars, with a redder hue, though there is some blue tint along the edges of the galaxy. There might be a faint disk component or some tidal features associated with the galaxy, but it is hard to tell with the resolution. There is no evidence of any major ongoing merger activity. Overall, the galaxy appears to be a relatively quiescent, evolved system.
