The galaxy appears to be a relatively smooth, elliptical-type galaxy. It exhibits a somewhat elongated, cigar-like shape, with a noticeable central bulge that appears brighter than the outer regions. The light distribution is fairly even across the galaxy, suggesting a lack of significant spiral arm structures or dust lanes. The color appears relatively uniform with a slight bias toward redder hues, which is consistent with an older stellar population. There is no visually obvious evidence of a recent major merger or significant tidal disturbances, although a minor disturbance or interaction cannot be completely ruled out based on this image alone. Overall, the galaxy presents as a well-formed, evolved system.
