The galaxy appears as a centrally concentrated object, exhibiting a dominant spheroidal morphology. There is a subtle disk-like structure that can be perceived, with the major axis of the disk oriented roughly horizontally in this view. The central bulge displays a yellowish hue, suggesting an older stellar population. The faint disk exhibits a bluer color gradient compared to the bulge, indicating the presence of younger, hotter stars and possibly ongoing star formation within the disk component.

Based on the subtle distortions and some of the clumpiness, the galaxy may be undergoing minor interactions or disturbances, although the overall structure is relatively unperturbed.
