The galaxy presents a somewhat disturbed morphology, appearing as a system undergoing or having recently undergone a merging event. A significant portion of the galaxy's light appears concentrated in a central region, suggesting a possible bulge component, although the resolution limits detailed examination. This central region exhibits a yellowish hue, potentially indicating an older stellar population. Extending from this central area, there are fainter, bluer patches, possibly indicative of regions of more recent star formation. An elongated feature is present that is much more red. The overall structure is not clearly defined as a spiral or elliptical, hinting at the possibility of an irregular or transitional type, which is consistent with a galaxy experiencing a dynamic interaction like a merger. 
