The galaxy presents as a mostly smooth, elliptical-like structure. There is a bright, concentrated central bulge that appears nearly spherical, with a gradually decreasing luminosity extending outwards. The overall color profile leans towards redder hues, particularly within the central region, suggesting an older stellar population with fewer hot, young stars. A slight extension of the galaxy is visible along one axis, deviating slightly from a perfectly circular shape. There is little evidence of prominent spiral arms or significant dust lanes, but subtle irregularities in the outer regions might indicate minor gravitational disturbances or tidal interactions with smaller companions. These faint disturbances could point to ongoing or past merger activity. The galaxy's smooth appearance implies that it has largely settled into a stable configuration.
