The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. The overall shape is round, showing minimal deviation from a circular morphology. There is a gradual decrease in luminosity from the core outwards. There are no visible spiral arm structures or indications of a prominent disk. The galaxy exhibits a yellowish-orange hue in the central region, suggesting an older stellar population, while the outer regions appear slightly bluer, potentially indicating a small amount of ongoing star formation. There is no evidence of major mergers or tidal disturbances, though a subtle asymmetry might suggest a minor interaction. The overall structure appears to be relatively undisturbed and quiescent.
