The galaxy presents a somewhat elliptical morphology. The central region exhibits a high surface brightness, suggesting a significant concentration of stars or an active galactic nucleus. A fainter, more diffuse halo surrounds the central bulge, extending further along the major axis of the ellipse. There is subtle evidence of a disk structure, but it is not sharply defined. Some faint features or irregularities are visible within the halo region, possibly indicative of minor tidal interactions or internal disturbances. Overall, the galaxy appears relatively smooth and undisturbed. The color gradient suggests a redder core region, potentially due to older stellar populations, with bluer hues in the outer regions, possibly indicating younger stars or ongoing star formation.
