The galaxy presents as a relatively compact and smooth object with a discernible core. Its color profile suggests a population of older stars, exhibiting a yellowish-orange hue, although there may be some pockets of active star formation as indicated by the presence of a central cyan region. The morphology is largely spheroidal, with a slight suggestion of elongation. There appear to be faint disturbances, suggesting some past interaction with another galaxy, but it does not seem to be currently undergoing a major merger.
