The galaxy presents as a relatively compact, elliptical-like structure. It exhibits a smooth, largely featureless appearance with a concentrated central region that decreases in intensity gradually. There are some subtle color gradients, with the central region appearing to exhibit a yellowish hue, potentially indicating an older stellar population. This central region is surrounded by a dimmer, redder halo, possibly due to older, cooler stars in the outer regions. There is no clear evidence of spiral arms or a distinct disk structure. The overall shape appears generally circular. There is no obvious tidal disturbance or ongoing merger event evident.
