The galaxy presents as a dominant, elliptical or lenticular structure with a smooth and largely featureless morphology. It exhibits a centrally concentrated light distribution that gradually decreases in intensity towards the outer regions. There is a subtle deviation from perfect circularity, with a possible slight elongation. The core appears relatively bright, with the overall color profile leaning towards the redder end of the spectrum, indicating an older stellar population and a low rate of ongoing star formation. There appears to be possible interactions with a very small dwarf galaxy. There seems to be some disturbances in the morphology, which could support it possibly merging.
