The galaxy appears as a flattened, elliptical structure, elongated along its major axis. The central bulge exhibits a smooth, concentrated distribution of light, suggesting a significant population of older stars. Extending outward from the bulge is a disk-like component, though it is less prominent and appears somewhat disturbed. The overall color of the galaxy is slightly reddish, which is consistent with galaxies with moderate star formation and an older stellar population. There may be evidence of tidal features, in the form of wisps of faint emission extending outward from the main body of the galaxy. These could be indicative of a past merger or gravitational interaction. The disk does not exhibit well-defined spiral arms. Overall, the galaxy seems to be relatively mature, with evidence for past or ongoing gravitational interactions.
