The galaxy presents a smooth, elliptical morphology with a noticeable central bulge. The color gradient suggests a stellar population that is primarily old, with a dominant reddish-orange hue concentrated towards the core. A faint, greenish halo surrounds the central region, potentially indicating a small degree of ongoing star formation or ionized gas. There is no strong evidence of spiral arms or a disk-like structure. The galaxy exhibits a slight elongation, appearing more oblate than perfectly spherical. There are no signs of tidal disturbances or ongoing mergers, indicating that the galaxy is relatively isolated and undisturbed. Overall, it appears to be a mature, relatively quiescent galaxy.
