The galaxy presents as a somewhat rounded, centrally concentrated object. Its color gradient suggests an older stellar population dominating its composition. There is little evidence of spiral arms or prominent dust lanes. The object appears largely smooth in texture, with a slight blue tint towards the edge. The overall shape is consistent with an elliptical galaxy or a lenticular galaxy viewed face-on. There is no obvious sign of any recent merger activity or major disturbances. The galaxy exhibits a concentrated central region suggesting the potential presence of a supermassive black hole. Star formation is either minimal or obscured. The structure implies a relatively evolved system, likely having exhausted much of its gas reservoir for star formation.
