The galaxy presents as a disturbed system, exhibiting signs of interaction or recent merger activity. The primary body of the galaxy shows a somewhat amorphous structure, lacking a well-defined spiral arm pattern or a dominant elliptical shape. There are visible color gradients across the galaxy; the core region appears relatively redder, suggestive of an older stellar population, while the outer regions display bluer hues, potentially indicating ongoing star formation. The galaxy exhibits a noticeable disruption in its morphology, possibly indicative of tidal forces at play. Faint extensions or plumes of material are seen, further supporting evidence of gravitational interaction. Overall, the galaxy appears to be in a state of flux, undergoing significant morphological transformation.
