The galaxy presents as a centrally concentrated object with a somewhat disturbed morphology. A pronounced bulge dominates the central region, appearing yellowish-white, suggesting an older stellar population. Fainter and bluer light is visible around this bulge, especially in the surrounding disk-like structure, implying ongoing or recent star formation. There's a hint of a spiral arm structure, though disrupted. Patches of redder regions can be seen within the disk, potentially indicating regions of dust obscuration or the presence of HII regions. The overall form of the galaxy leans towards intermediate classifications, blurring the lines between pure elliptical and spiral characteristics. A slight asymmetry in the outer disk is observed, possibly caused by an interaction. The galaxy does not seem to be actively undergoing a major merger.
