The galaxy appears relatively compact, with a bright, concentrated central region. There is some indication of a more extended, diffuse halo surrounding the core, though this is faint and somewhat irregular in shape. Color gradients are present; the central region displays a bluer hue, suggesting the presence of younger, hotter stars or active galactic nucleus activity. Moving outward, the color shifts toward a greener tone, possibly indicating a population of older stars or a lower rate of star formation. Subtle irregularities are visible in the outer regions of the galaxy, with hints of asymmetry suggesting possible minor tidal disturbances or interactions. Overall, it seems to be relatively elliptical in shape.
