The galaxy exhibits an elongated morphology with an apparent major axis of approximately 10 arcseconds. The central region is dominated by two bright, unresolved cores, suggesting the possibility of a recent or ongoing merger event. There is a diffuse halo surrounding the central cores, which appears to be composed of older stellar populations, judging by its reddish hue. This halo shows some tidal features, with faint extensions visible which could indicate gravitational interactions. No clear spiral arm structure is evident. The overall color profile suggests a mix of stellar ages, with the central cores possibly hosting younger, bluer stars, while the outer regions appear redder. The galaxy exhibits an irregular structure, possibly indicative of morphological disturbance.
