The galaxy presents as an elliptical-like structure with a bright, concentrated central bulge. The overall color appears yellowish-white, suggesting a relatively older stellar population within the bulge. The outer regions of the galaxy exhibit a fainter and bluer hue, possibly indicating the presence of younger stars or regions of recent star formation, although the lack of distinct spiral arms is notable. The galaxy appears to be relatively smooth in texture with no obvious signs of significant disturbances or major mergers. Its shape shows a degree of flattening, presenting an oval appearance from our observational perspective. There may be slight asymmetries or irregularities in the distribution of the outer light, suggesting potential minor interactions or ongoing accretion events.
