This galaxy presents as a relatively smooth, somewhat rounded object. The core region exhibits a concentrated, bright luminosity, suggesting a substantial population of older stars or possible AGN activity. The overall color is yellowish-orange, indicative of an older stellar population with lower rates of current star formation. There is a slight asymmetry in its morphology, perhaps a minor disturbance on the right side of the core, which might indicate a tidal interaction or a minor merger event. Although diffuse, the galaxy appears to be generally well-defined.
