The galaxy presents as a relatively smooth, elliptical-like object with a centrally concentrated brightness profile. It exhibits a radial gradient in luminosity, with the core appearing significantly brighter and more yellow than the diffuse outer regions. The galaxy appears to be mostly undisturbed, without any major signs of tidal interactions or ongoing mergers. The overall color suggests an older stellar population. The apparent lack of significant dust lanes or spiral arm structures further supports a classification leaning towards an early-type galaxy.
