The galaxy appears to be a luminous, relatively compact system with a smooth and rounded morphology. It exhibits a concentrated central region, likely indicative of a bulge component. The overall color profile suggests a population of older stars, although bluer tinges are slightly visible. There's no prominent spiral arm structure or distinct features to indicate ongoing major star formation throughout the galaxy, however low levels are likely. There are subtle asymmetries present in the outer regions, suggesting a possible minor disturbance or past interaction, but it appears mostly undisturbed. The object is not undergoing any major merging activity. The galaxy exhibits a general shape that could be classified as elliptical, without a pronounced disk-like structure.
