The galaxy presents as a relatively smooth, elliptical-like structure. There is a central, bright core region that decreases in luminosity as it extends outwards. The color profile suggests a population of older stars with an average magnitude, with minimal indication of active star formation. The galaxy exhibits a primarily homogenous structure, exhibiting no notable spiral arm morphology or significant dust lane obscuration. Its overall shape is somewhat round with only minor disturbances. No merging events or major interactions appear to be taking place.
