The galaxy presents a generally smooth and rounded morphology. The central region exhibits a concentrated luminosity, appearing bright yellow. This suggests a population of older stars. There is a slight elongation, but the overall shape is fairly symmetrical. No prominent spiral arms or bar structures are discernible. The outer regions of the galaxy appear fainter and bluer, indicating the possible presence of younger stars or ongoing star formation, although at a seemingly low rate. The overall structure appears relatively undisturbed, exhibiting no significant signs of ongoing or recent major merger activity. There is only a slight asymmetry, but this could be explained by the presence of dust obscuring some of the galaxy. The galaxy is an elliptical galaxy.
