The galaxy appears to be a relatively smooth, elliptical type. It exhibits a centrally concentrated bulge with a gradual falloff in luminosity towards the outer regions. The color gradient suggests a possible radial change in stellar population, with a more reddish hue at the core transitioning to slightly bluer tones further out. There is no obvious indication of spiral arms or significant dust lanes. The overall morphology indicates it is undisturbed, with no signs of major tidal interactions or recent mergers. The galaxy is quite compact.
