The galaxy appears to be a relatively small, elliptical system. It exhibits a smooth, concentrated light profile, with the highest intensity at the core. The overall shape is elongated, resembling a cigar shape. There appears to be no significant spiral arm structure, distinct bar, or prominent dust lanes. A slight distortion may be present in the galaxy's outer isophotes. There is little evidence of major mergers or significant tidal disturbances, though subtle irregularities can be observed. The system's color suggests an older stellar population, possibly with a lack of ongoing star formation.
