The galaxy appears as a smooth, elliptical-like structure, exhibiting a concentrated central bulge. Its overall shape is somewhat elongated, possibly leaning toward a cigar shape, but is still largely considered to be in between elliptical and cigar-shaped. The galaxy's color profile indicates an older stellar population, with a yellow-orange hue dominating the observed light. There is little evidence of spiral arms or significant dust lanes. The system exhibits no strong signs of tidal disturbances or ongoing major merger activity, but there may be some signs of a minor disturbance or a recent minor merger. 