The galaxy presents a largely smooth morphology, with little to no discernible spiral structure or prominent features. The light is concentrated centrally, suggesting a significant bulge component. The overall shape appears elliptical, trending towards a slightly elongated, but not significantly cigar-shaped, form. There is no obvious evidence of ongoing mergers or major disturbances; the galaxy appears relatively undisturbed. The color profile indicates a population of older stars, seen by the redder hue of the outer regions of the galaxy, with a slightly bluer, more actively star-forming core. There is a clear dropoff in brightness and change in color as we move from the center, suggesting a gradual transition from the bulge to the outer halo.
