The galaxy presents as a lenticular, cigar-shaped structure with a smooth, diffuse light profile. A slight color gradient is observed, trending towards bluer hues at the apparent edges of the galaxy. There is a faint, distorted structure extending from one end, possibly indicative of tidal interactions. A minor disturbance cannot be ruled out. The object exhibits a moderately low star formation rate, suggesting a primarily aging stellar population. The overall mass appears relatively modest.