The galaxy presents a smooth, elliptical morphology with a concentrated central bulge. The color appears generally yellow, with a slightly redder core, suggesting an older stellar population. There is little evidence of spiral arms or significant dust lanes. The galaxy exhibits a generally rounded shape, with only a slight elongation. There is no strong visual indication of any ongoing mergers or major disturbances affecting the galaxy's structure. The galaxy appears relatively isolated within the observed field, with no nearby companions apparently gravitationally interacting.
