The galaxy appears to be a relatively smooth, elliptical type. The light profile exhibits a centrally concentrated bulge that fades gradually towards the edges. There is little evidence of spiral arm structure or significant dust lanes. The galaxy has a slightly elongated shape, and a fraction of the light appears to be concentrated in a slightly cigar shape. The colour is generally yellowish-white, consistent with an older stellar population. No signs of ongoing major mergers or significant tidal disturbances are apparent. There may be hints of a faint disk or subtle features.