The galaxy presents as a somewhat irregular structure, potentially indicative of a disk galaxy with some level of disturbance. It exhibits a core region with a high degree of central concentration that shows a bluish-white hue, likely suggesting the presence of younger stellar populations and ongoing star formation. The overall morphology suggests a transition from a smooth, elliptical galaxy to a more structured, spiral-like galaxy. There's an area to the side of the galaxy, with a yellow hue, suggesting an area of high concentration of older stars. The features observed suggest a recent merger or tidal interaction is also possible.
