The galaxy appears as a relatively smooth, elliptical object with a concentrated central bulge. The light distribution suggests a high degree of radial symmetry, with a gradual decrease in intensity from the center outwards. There is a subtle color gradient, with the central region exhibiting a slightly yellower hue, possibly indicative of an older stellar population, while the outer regions appear slightly bluer, suggesting ongoing or recent star formation activity. No distinct spiral arms or prominent dust lanes are discernible. The overall morphology suggests a system that has undergone significant dynamical relaxation and aging. There may be an interacting object nearby which could contribute to the increased star formation.
