The galaxy appears to be an interacting system of galaxies, with a larger, relatively smooth elliptical galaxy interacting with a smaller, disrupted spiral or irregular galaxy. The elliptical component exhibits a high degree of sphericity, with a smooth light distribution and a slight elongation. It presents a dominant central core. The secondary galaxy displays a disturbed morphology, characterized by a flattened disk, irregular shape and diffuse outer region. The color distribution suggests ongoing star formation within both galaxies. The smaller galaxy displays bluer colors than the elliptical component, with possible localized pockets of intense star formation. Both galaxies appear to be gravitationally bound. There are signs of tidal interactions, the smaller galaxy appears to have a tail and the elliptical galaxy appears to have a faint halo. Overall, this galaxy presents a complex structure resulting from galaxy interactions or a possible merger.
