The galaxy presents as a generally elliptical structure, with a bright, concentrated central region which fades radially outwards. The central luminosity suggests a significant concentration of stars, potentially indicating the presence of a supermassive black hole. The outer regions of the galaxy display a diffuse, disk-like structure with some irregularities. Evidence of a faint, incomplete ring structure is observed, suggesting a prior minor merger. There are no apparent spiral arms or prominent dust lanes visible. The overall color of the galaxy suggests a population of relatively older stars, with a possible recent starburst in the center.
