The galaxy presents as a complex system, possibly undergoing a merger or exhibiting strong tidal interactions. There is evidence of significant disturbance to the primary galactic structure. At least two distinct nuclei are observed, suggesting the presence of multiple interacting galaxies or a single galaxy with a highly disturbed core.

The morphology appears neither purely elliptical nor a well-defined spiral. There's a diffuse component surrounding what seems to be the main body, indicating a possible tidal tail or disrupted disk. The light distribution is uneven, showing concentrations of brighter regions interspersed with fainter areas.

Based on the color profile, there appear to be areas of active star formation, indicated by the bluer hues in some regions, while other areas show redder colors, which may indicate older stellar populations or dust obscuration. Overall, the galaxy is far from a relaxed state, hinting at dynamic processes reshaping its structure.
