The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. There is no clear evidence of spiral arms or a distinct disk. It is primarily yellowish in the center, suggesting an older stellar population dominating the core. Fainter bluish and greenish hues are observed in the outer regions, indicating the possible presence of younger stars or star-forming regions, although these are not prominent. The overall morphology appears undisturbed; there are no obvious signs of a recent major merger or tidal disruptions. The axial ratio suggests a slightly elongated, rather than perfectly circular, shape.
