The galaxy appears as a concentrated, centrally brightened structure with a relatively smooth overall morphology. The core region exhibits a yellowish-white hue, suggesting a population of older stars. The outer regions gradually fade in intensity, with a subtle reddish component observable in the surrounding halo. No distinct spiral arms or prominent dust lanes are visible. The galaxy demonstrates a mildly elliptical shape, and is relatively compact. Based on the available visual information, this galaxy may represent an elliptical morphology, likely composed of a considerable number of stars.
