The galaxy presents a generally smooth, elliptical morphology. It appears relatively undisturbed, showing no strong visual evidence of ongoing major merger activity or significant tidal features. The light distribution is concentrated towards the center, with a gradual decline in intensity moving outwards. The galaxy exhibits a dominant red color profile, with some indication of a bluer component particularly in the inner region. The overall color suggests a population of older stars with moderate ongoing star formation. The apparent roundness and smooth profile suggests a galaxy with minimal visible disk structure.
