The galaxy presents as a centrally concentrated, elliptical morphology with a smooth light distribution. The core exhibits a bright, yellowish-white hue, indicative of an older stellar population. The galaxy lacks any readily discernible spiral arm structure or prominent dust lanes. The outer regions display a gradual fading of light intensity, transitioning into a diffuse halo. There's a slight elongation present, deviating marginally from a perfectly circular shape. No obvious signs of tidal interactions or major mergers are visible, although subtle disturbances cannot be ruled out without higher resolution data. The galaxy appears relatively isolated.
