The galaxy presents as a centrally concentrated object with a smooth morphology. It exhibits a slightly elliptical shape and appears to lack significant spiral arm structures or prominent dust lanes. Its color profile suggests a population of older stars, potentially indicating relatively low current star formation. There is some slight asymmetry visible in the outer regions of the galaxy which may be due to a minor disturbance, but it largely appears undisturbed. It presents no signs of an ongoing major merger.