The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a largely elliptical morphology, displaying a high degree of radial symmetry, with a hint of a disk. The core appears luminous, decreasing in intensity towards the outer regions. There is no evidence of strong spiral arm structures or prominent dust lanes. The overall color profile indicates a population dominated by older stars, with minimal signatures of ongoing, active star formation. There are hints of a minor disturbance in morphology but it is not overtly undergoing a merging event. 
