The galaxy exhibits a generally smooth morphology, with a dominant central bulge. A slight asymmetry is present in the outer regions, possibly indicative of a minor gravitational interaction or past merger event. The core appears bright, potentially signifying active star formation or an active galactic nucleus. The object displays a primarily spherical shape, with a subtle elongation along one axis. Color gradients are evident, with a bluer hue concentrated in the central region, suggesting a population of younger, hotter stars. Redder tones are observed in the outer halo, indicative of older stellar populations. Patches of less dense material exist on the fringes, hinting at tidal debris or disrupted structures.
