The galaxy presents an irregular morphology. Its light profile suggests a relatively compact object, appearing somewhat diffuse. There is no clear spiral arm structure or prominent central bulge visible. Evidence suggests possible interactions or disturbances, with hints of asymmetry and faint, extended features that may indicate tidal tails or disrupted components resulting from a merger event, potentially minor or major in scale. The central region displays a higher surface brightness compared to the outer regions, which fade into the background. The overall color appears to be fairly uniform.
