The galaxy appears to be a relatively smooth, centrally concentrated system. Its overall color is yellowish-orange, hinting at a somewhat older stellar population with fewer hot, young stars. While the bulk of the galaxy is smooth, there is subtle evidence of faint, diffuse, greenish outer regions, which could potentially indicate some recent or ongoing star formation, though at a low level. There is also a hint of a minor disturbance on the bottom-right side of the galaxy. The primary morphology is elliptical or lenticular, with no obvious spiral arm structure visible. The galaxy appears roughly circular, with a slight tendency towards being in between round and cigar-shaped. There may be some evidence that the galaxy could be in the process of merging.
