The galaxy exhibits a disturbed morphology, potentially indicative of an ongoing or recent merger event. A significant portion of the galaxy's light appears concentrated within a bright, central region. This core shows a yellowish-white hue, which could suggest an older stellar population or significant dust obscuration. Extensions emanate outwards, exhibiting a bluer color. The galaxy's overall shape departs substantially from a regular elliptical or spiral form. Faint, diffuse components are present, indicating a relatively extended halo or tidal features resulting from gravitational interactions. The galaxy appears at an approximate redshift of 0.29.
