The galaxy presents as a disturbed system, likely undergoing a merging event. Two distinct luminous cores are observed, suggesting the presence of two interacting galaxies. One core appears more spherical and compact, exhibiting a yellowish hue. The second core is slightly elongated, with some evidence of tidal features extending outwards. The overall color profile indicates a mature stellar population, although the bluer tones in some regions hint at ongoing star formation. The morphology is irregular, lacking a defined spiral or elliptical structure. The galaxy system appears to be significantly perturbed from a relaxed state, possibly indicating late stage of an ongoing merger event.
