The galaxy presents a predominantly smooth morphology with a bright, concentrated central bulge. The overall shape appears elliptical, tending towards a circular form rather than a highly elongated or cigar-like structure. There is no strong evidence of spiral arms or a distinct disk. Faint diffuse light extends outwards from the central region, suggesting a halo of stars or dust. There is a subtle color gradient observable, transitioning from a slightly bluer hue in the outer regions to a warmer, yellow-orange tone toward the core. No major signs of ongoing mergers or tidal disturbances are apparent, although minor irregularities might be present but are difficult to resolve given the image quality.
