This galaxy exhibits a disturbed morphology. There is evidence of a possible ongoing or recent merger event, indicated by asymmetrical features and potential tidal distortions. The galaxy appears to have a central concentration of light, but lacks a well-defined, smooth structure, with diffuse and irregular components throughout. Patches of bluer light suggest regions of ongoing star formation, intermixed with areas of redder light, consistent with an older stellar population. Overall, the galaxy is relatively compact, appearing as a moderate sized structure with hints of features suggesting ongoing interactions or internal disturbances.
