The galaxy appears to be a relatively smooth, elliptical galaxy. Its central bulge is bright and concentrated, with a yellowish-white hue, suggesting an older stellar population. The outer regions of the galaxy fade gradually, exhibiting a slightly bluer tint, possibly indicating the presence of younger stars, or at least a less evolved stellar population than that in the bulge. The galaxy exhibits a somewhat rounded shape, though not perfectly circular. There is no clear evidence of a prominent disk or spiral structure. No significant tidal tails or major distortions are apparent, suggesting that this galaxy has not experienced a major merger recently, though some minor irregularities in the light distribution cannot be ruled out.
