The galaxy presents as a generally smooth object, exhibiting a concentrated central bulge. There is no discernable spiral structure, nor is there any obvious bar feature. The color profile suggests an older stellar population, appearing more yellow-red. It is relatively compact, appearing circular. There are no obvious tidal tails or shell structures indicative of a recent major merger event, however a very slight asymmetry might suggest a minor gravitational interaction. There may be a faint, very diffuse disk component.
