The galaxy presents as a relatively smooth, elliptical-like structure, with a concentration of light towards the center indicative of a prominent galactic bulge. Its shape appears mostly round, though subtle deviations may be present. There is a very slight suggestion of a faint, diffuse halo surrounding the main body of the galaxy. The color profile suggests a population of older stars, implying that the galaxy is not undergoing significant star formation currently. There is no evidence of spiral arms or a disk-like structure. No major merger events are apparent, with no significant tidal tails or disturbed morphology.
