The galaxy presents as a generally smooth, elliptical-like structure with a concentrated central bulge. The light distribution appears relatively uniform across the main body, with a noticeable radial decrease in luminosity moving outward from the core. There is a slight elongation in the morphology. Some subtle irregularities or minor disturbances are possibly present in the outer regions, hinting at past or ongoing interactions. The color profile suggests a significant population of older stars, indicated by the yellowish hue, which could also indicate substantial dust extinction. There is no prominent spiral arm structure or significant regions of active star formation clearly visible in this imagery.
