The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The color profile suggests a population of older stars, with a dominant yellowish-red hue in the core, transitioning to a slightly bluer tint in the outer regions. There is little to no evidence of spiral arms or dust lanes. The overall light distribution indicates a fairly even stellar density, with a gradual falloff from the center outwards. Minor asymmetry can be observed, though the galaxy is not undergoing any major mergers.
