The galaxy presents as a relatively smooth, elliptical structure. It exhibits a moderate degree of ellipticity, appearing elongated rather than perfectly spherical, approaching a cigar-like shape. The light distribution is concentrated toward the center, with a bright central bulge region displaying a reddish hue. This suggests a higher concentration of older stellar populations in the core. Moving outward from the core, the galaxy displays a gradual decrease in brightness. The outer regions exhibit a more greenish-yellow color gradient, suggestive of more recent star formation and younger stellar populations, although the presence of distinct spiral arms is not evident. The overall morphology indicates a lack of significant ongoing mergers or major disturbances. There is no evidence of tidal tails, bridges, or other signatures of recent gravitational interaction. Based on its smooth morphology, the galaxy is likely an elliptical galaxy.
