The galaxy presents a predominantly smooth morphology, appearing as an elliptical-like structure. A central, bright bulge dominates the galaxy's core, with a diffuse halo extending outwards. There's a hint of a disk-like structure, with a slight elongation visible. No spiral arms are clearly discerned. The overall color suggests a population of older stars, with a subtle bluer hue in the outer regions potentially indicating some ongoing star formation. There are no distinct signs of a major ongoing merger or tidal disturbances, though some minor irregularities in the halo region cannot be excluded. The galaxy's light distribution appears quite concentrated, with a high Sersic index pointing to an elliptical morphology.
