The galaxy presents as a largely smooth, centrally concentrated object. Its overall color appears yellowish-orange, suggesting a stellar population dominated by older, redder stars. The galaxy exhibits a generally round morphology, with minimal deviation from circularity. There is no apparent evidence of significant tidal features, strong spiral arms, or a prominent bar structure. The lack of clear substructure or irregularities indicates that it has not recently undergone a major merger event, although a minor disturbance cannot be ruled out. Overall, the galaxy appears to be a relatively undisturbed, mature system.
