The galaxy presents a largely featureless, smooth morphology. The central region exhibits a high degree of luminosity, suggesting a concentrated stellar population or potentially an active galactic nucleus. This bright core gradually fades into a more diffuse halo or bulge component. The overall shape appears to be elliptical or spheroidal, with no readily apparent spiral arm structures or a distinct disk. There is a slight elongation, but the galaxy is generally rounded. No significant signs of ongoing mergers or tidal disturbances are visible. Color gradients are subtle; the central region appears slightly yellower, possibly indicating an older stellar population, transitioning to bluer hues in the outer regions, suggesting more recent star formation.
