The galaxy presents as a fairly symmetrical elliptical or lenticular morphology. It exhibits a smooth luminosity profile, with a concentrated central bulge that gradually fades into the outer regions. There is minimal evidence of spiral arm structure or prominent dust lanes. The color appears slightly redder, suggesting an older stellar population with fewer young, massive stars. The galaxy appears relatively isolated, with no obvious signs of tidal interactions or ongoing mergers. Given its apparent size and morphology, it likely constitutes a massive galaxy.
