The galaxy presents a generally smooth, elongated morphology, appearing cigar-shaped. The central region is notably brighter and exhibits a yellowish-white hue, suggesting a concentration of older stellar populations. Moving outwards from the core, the galaxy exhibits a gradual decrease in luminosity. There is the suggestion of a diffuse disk surrounding the central bulge; however, the disk appears relatively featureless with no readily discernible spiral arms. The overall color gradient indicates a potential lack of significant ongoing star formation, although a low level of activity cannot be ruled out based on this imagery alone. Signs of any major disturbances or ongoing mergers appear minimal.
