The galaxy appears to be relatively compact, with a somewhat amorphous structure. The central region displays a bright, concentrated core. A slight elongation is noticeable, deviating from a perfectly circular morphology. There is evidence of a possible interaction or disturbance, indicated by an irregular extension or plume emanating from one side of the central region, creating an asymmetric profile. Color variations suggest differential stellar populations or dust distribution. The central core exhibits a bluish hue, potentially indicating younger, hotter stars, while the outer regions and the extended feature show hints of redder colors, possibly due to older stellar populations or dust reddening. Overall, the galaxy appears to be in a state of moderate activity, with hints of ongoing or recent interactions influencing its morphology and star formation.
