The galaxy presents as a merging system or a galaxy experiencing significant tidal disruption. The core region appears complex, with two particularly bright, compact components suggestive of interacting galactic nuclei or regions of intense star formation triggered by a merger event. These bright cores are embedded within a more diffuse, irregular halo of light. The overall morphology suggests a dynamic and gravitationally disturbed system, rather than a well-defined spiral or elliptical galaxy. There is evidence of lower surface brightness material extending beyond the central region, hinting at tidal tails or other debris resulting from the interaction. The color profile suggests a mixed stellar population, with both older, redder stars and potentially younger, bluer stars contributing to the overall light.
