The galaxy exhibits a distorted morphology, suggestive of an ongoing or recent interaction. It displays an elliptical-like structure, with an asymmetric distribution of light. There is evidence of tidal tails or extended features emanating from the main galactic body. The central region appears relatively smooth and concentrated, while the outer regions show a more diffuse and irregular structure. Color variations are apparent, with a reddish hue in some areas and bluer tones in others, potentially indicating differing stellar populations and star formation activity. Overall, the galaxy appears to be dynamically disturbed, deviating from a regular spiral or elliptical form.
