The galaxy presents as two distinct components, suggesting a possible interaction or merger. The larger, more dominant component appears relatively smooth and elliptical in shape. Its light distribution is concentrated toward the center, with a gradual falloff in intensity towards the edges. There is a slight color gradient, with the central region appearing more yellow, indicating an older stellar population.

The second component, located slightly offset from the main body, is smaller and exhibits a more elongated, disk-like structure. It displays bluer colors compared to the larger component, potentially indicative of ongoing star formation. There are some signs of possible tidal disturbance or disruption, though these are not highly pronounced.

The overall appearance of the system points to a moderately massive galaxy at a considerable distance, with moderate star formation activity occurring primarily in the smaller, disk-like companion or region. The relative smoothness of the main galaxy and the apparent interaction suggest it could be evolving towards an elliptical morphology.
