The galaxy appears as a relatively smooth, elliptical object. It exhibits a concentrated central bulge with a diffuse halo extending outwards. There is no clear spiral arm structure visible. The color gradient suggests a population of older stars, with a yellowish hue dominating the central regions. The outskirts appear slightly bluer, which could indicate the presence of younger stellar populations, however the general color indicates that is it a red and dead galaxy. No significant dust lanes or active star-forming regions are discernible in this image. The galaxy seems to be relatively isolated, displaying no obvious signs of ongoing or recent major merger events, although a possible minor interaction with a nearby object may exist to the lower left. The overall morphology suggests a galaxy nearing the end of its star formation activity.