This galaxy appears as a slightly elliptical object. Its structure is largely smooth and concentrated, displaying a mostly homogenous profile without prominent spiral arms or a distinct bar. The overall color suggests a population dominated by older stars, possibly implying a relatively low current star formation rate. A subtle color gradient exists moving outwards from the center, which could be indicative of varying stellar populations and ages within the galaxy. There is a hint of potential disturbance, possibly related to a minor interaction or past merger event influencing its shape.
