The galaxy presents as a roughly elliptical structure, exhibiting a smooth, centrally concentrated light profile. The core region displays a bright, yellowish-white hue, suggesting a population of older stars. Moving outward from the core, the color transitions slightly to a bluer tint in the surrounding disk, possibly indicating the presence of some younger stars and regions of moderate star formation activity. There are faint hints of spiral arm structures but they are hard to discern due to the rounder nature of the galaxy. No significant dust lanes or prominent star-forming regions are immediately apparent. There is no obvious ongoing major merger event, although minor tidal disturbances may not be ruled out based on this image alone. The overall morphology leans towards an early-type spiral or a lenticular galaxy, given the smooth, centrally concentrated light profile.