The galaxy presents as a relatively compact object. It exhibits a subtle elongation, suggesting a possible disk-like structure. The color appears predominantly reddish, with slight variations in intensity across the galactic body. A low surface brightness suggests this galaxy is either faint or distant. The overall morphology appears disrupted, possibly indicating an interaction with another galaxy, or it could simply be an irregular galaxy. There is evidence of a slight tidal tail, further suggesting a past or ongoing merger event. The core appears somewhat indistinct, lacking a clearly defined central bulge. This might indicate a lower mass or more diffuse distribution of stars in the galaxy's central region. The galaxy's structure and the faint tidal tail seem to support a potential classification as an irregular or merging galaxy. Higher resolution imaging or spectroscopic data would be beneficial to confirm its exact morphological type and further characterize the nature of the disruption.
