The galaxy presents as a largely featureless, elliptical-like structure. Its overall morphology appears smooth, with a high degree of central concentration. The light distribution is relatively even, displaying a gradual decline in intensity from the core to the outer regions. There is little to no apparent structure indicative of spiral arms or a prominent disk component. The galaxy exhibits a yellowish hue, suggesting a stellar population dominated by older stars. The galaxy appears fairly isolated, with no obvious signs of tidal interactions or ongoing mergers. The morphology suggests it is a mature system which has experienced any recent major merger events.