The galaxy presents as a slightly elongated spheroid with a concentrated central bulge. The color is predominantly yellow-orange, suggesting an older stellar population with fewer young, hot, blue stars. There is a notable absence of spiral arm structures or significant dust lanes, and the smooth light distribution indicates that this galaxy is an elliptical. The outer regions of the galaxy gradually fade into the background sky, suggesting a diffuse halo. There is no apparent major morphological disturbance due to mergers or interactions, though I observe a second galaxy in the upper-right that may be gravitationally interacting.
