The galaxy presents as an elliptical morphology, appearing largely smooth and spheroidal. Its core region exhibits a bright, concentrated intensity, suggesting a high stellar density. The radial color profile indicates a gradual transition from a yellow-orange core to a bluer outer halo. There are no visually identifiable spiral arms or distinct dust lanes. The overall structure appears undisturbed, with no obvious signs of recent major merger activity or tidal interactions. The galaxy appears relatively isolated within its field.
