The galaxy appears to be a relatively smooth, elliptical-like structure, though not perfectly spherical. The light is concentrated in the center and fades gradually toward the edges. It presents a yellowish hue, which might indicate an older stellar population with fewer young, hot stars. There is no obvious spiral arm structure or prominent dust lanes. There might be a very slight elongation but this is not well defined from the source. The galaxy appears relatively undisturbed, with no major signs of ongoing mergers or tidal distortions. The overall impression is that of a relatively massive, evolved galaxy at a considerable distance.
