The galaxy appears as a single, unresolved object with a noticeable deviation from perfect circularity. There's an apparent elongation, suggestive of an intermediate shape between round and cigar-like. The object displays a color gradient, appearing bluer in the central regions and transitioning to redder hues in the outer regions. This could indicate the presence of younger, hotter stars concentrated towards the core, with older, cooler stars populating the periphery. There are clear signs of tidal interactions and merger activity, perhaps a small disturbance or a past merger event. There are also slight hints of a disk feature that could be causing some of the distortion of the overall form.
