The galaxy presents as an elliptical morphology, with a smooth and relatively featureless appearance. The light profile appears centrally concentrated with a gradual decrease in intensity outward from the core. The galaxy exhibits a moderate ellipticity, appearing somewhat elongated rather than perfectly circular. The color index suggests a population dominated by older stars, indicated by the overall reddish-yellow hue. There is no discernible evidence of spiral arms, dust lanes, or active star-forming regions. There appear to be no indications of any major ongoing or recent merger events. Minor disturbances are possible, but not highly evident.
