The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated central bulge, with a gradual decrease in luminosity outwards. There is little to no evidence of spiral arm structure or prominent dust lanes. The galaxy's color is somewhat uniform across its extent, suggesting an older stellar population. The roundness of the galaxy indicates minimal distortion or interaction with other galaxies, with no indication of tidal tails or other disturbances. The morphology of the galaxy suggests it is a fairly evolved system.
