The galaxy presents a largely smooth and elliptical morphology. It exhibits a bright, concentrated central bulge, transitioning to a fainter, diffuse halo. The shape is somewhat elongated, appearing more cigar-shaped than perfectly spherical. There is no readily apparent evidence of spiral arms or significant disk structure. The galaxy displays a color gradient, with the central region appearing more yellow, possibly indicating an older stellar population, while the outer regions exhibit a slightly bluer hue, suggestive of ongoing, though modest, star formation activity. There is no clear indication of any major merger events or tidal disturbances affecting its overall structure, although minor irregularities cannot be ruled out at this resolution.
