The galaxy presents as a slightly disturbed, elliptical morphology. A smooth, centrally concentrated spheroid is evident, with hints of asymmetry possibly due to interactions or minor merging events. There appears to be a brighter core, indicating a high concentration of older stars and potentially a supermassive black hole. The overall color suggests an older stellar population, with a redder hue. There is a possibility of some tidal disturbances or faint features, but they appear poorly defined and may just be noise.
