The galaxy exhibits a generally smooth morphology, with a centrally concentrated light distribution. It appears elongated, presenting an oblate spheroidal shape. The color profile suggests a population of older stars, with a redder hue dominating the overall appearance. There is some indication of a disk structure, but this is not as prominent as the central bulge. No significant tidal features or major disturbances are apparent, implying that it may have undergone relatively quiescent evolution.
