The galaxy presents as a centrally concentrated object, generally smooth in appearance. Its morphology suggests a lack of significant spiral arms or prominent disk features. The light distribution is dominated by a core brightness which fades smoothly outward in a roughly circular fashion. The overall color profile appears to be relatively uniform across the galaxy, trending toward the redder end of the spectrum, possibly indicating an older stellar population. There is no apparent distortion or asymmetry in the galactic structure, suggesting it is relatively undisturbed and not currently undergoing any major merging events. Based on its overall form and color, this galaxy may be classified as an elliptical or lenticular galaxy.
