The galaxy presents a nearly elliptical morphology, exhibiting a smooth, concentrated light distribution characteristic of an early-type galaxy. The light is centrally concentrated, with a gradual decrease in intensity outwards from the core. The galaxy appears largely featureless, lacking prominent spiral arms or distinct dust lanes. There are no signs of recent merger activity. The observed color profile suggests a population of older stars, with a subtle color gradient from a slightly more yellow/orange center to a bluer outer region. The galaxy is relatively compact and small.
