The galaxy exhibits a generally smooth morphology with some indications of internal structure. A bright, concentrated central region dominates the galaxy's luminosity, suggesting the presence of a galactic nucleus, possibly hosting a supermassive black hole. A faint, diffuse halo or disk-like structure surrounds the central bulge. This outer region shows slight irregularities, potentially indicating minor disturbances. There may be a small merger or the result of tidal interactions. The central region shows a bluer tint compared to the halo, which appears more red, potentially indicating differences in stellar populations or dust content.
