The galaxy presents as a generally smooth, elliptical-like structure. The central region exhibits a concentrated, bright core, potentially indicative of an active galactic nucleus or a dense stellar population. A diffuse, extended halo surrounds the core, gradually fading into the background. The color profile suggests a population of older stars, contributing to the galaxy's reddish hue in the central region. There are no apparent spiral arms or distinct dust lanes visible in the image, supporting the classification as a smooth galaxy. There are no signs of any ongoing major merger events. There may be a very slight disturbance or minor merger event occuring, but not enough to disturb the overall morphology of the galaxy. The galaxy appears mostly round in shape.
