The galaxy presents as an object with both smooth and featured characteristics. A central, moderately bright region exhibits a relatively smooth, condensed appearance, possibly indicating a bulge or core component. Extending outwards from this central region, fainter features suggest the presence of a disk. These features appear somewhat irregular, potentially indicative of ongoing gravitational interactions or internal disturbances. Faint patches of redder hue are observed in the galaxy's outer regions, possibly associated with star formation or dust. There is also a clear disturbance or plume of material extending away from the main body of the galaxy. The plume has a different color profile than the rest of the galaxy. This morphology may be the result of an ongoing merger. 
