This galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. The light distribution indicates a dominance of older stellar populations, suggested by the reddish-yellow hue, particularly concentrated in the core. There is a subtle color gradient observed, with the central region exhibiting a slightly more yellow tone compared to the outer regions that appear more red, suggesting a slight variation in stellar population or dust content. The galaxy shows no obvious signs of spiral arms, strong dust lanes, or significant ongoing star formation. The overall structure is relatively undisturbed, showing no major tidal features or morphological irregularities indicative of recent major mergers. The shape is moderately elliptical. There is very faint evidence of a disk, with minimal evidence of spiral arms, and appears to be largely quiescent in terms of star formation.
