The galaxy presents as a generally smooth, elliptical-like structure with a subtle central bulge. A slight disk feature is suspected, but not distinctly resolved. The light distribution appears moderately concentrated, transitioning smoothly from the core outward. The core exhibits a warm hue, potentially indicating a population of older stars. Some bluer tinges are observed in the surrounding areas suggesting on-going or recent star formation. There is no apparent morphological distortion, and it does not seem to be undergoing any major merging activity. Faint disturbances might be present but they are not conclusive.
