The galaxy presents as a centrally concentrated system with a smooth, diffuse light distribution, suggesting a significant spheroidal component. The primary color is a yellowish-white hue, indicative of an older stellar population, although bluer tinges can be seen at the outer edges of the disk. There is no discernible spiral arm structure or dust lanes within the galaxy's disk. There is evidence of some disturbances nearby, but no major merger apparent in this image.
