The galaxy appears to be a luminous, centrally concentrated object. It presents a somewhat elliptical morphology, although the resolution limits detailed shape characterization. A dominant, smooth bulge component is apparent, exhibiting a yellowish hue, potentially indicative of an older stellar population. Fainter, bluer regions are asymmetrically distributed around the central bulge, suggesting the presence of some star formation activity. There seems to be a hint of a disk-like structure, but it's difficult to tell for sure. There may be some minor disturbances in the overall structure suggesting a past or ongoing interaction.
