The galaxy appears to be a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge with a yellowish hue, suggesting an older stellar population dominating the core. The outer regions display a bluer color, possibly indicating the presence of younger stars or ongoing star formation, albeit at a low rate. There is a lack of clearly defined spiral arms or prominent dust lanes, further supporting the classification of a possible elliptical or lenticular galaxy type. The galaxy appears somewhat elongated. There is no evidence of major mergers or tidal disturbances in this image, although there may be some minor interaction occurring.
