Observed galaxy appears to be part of an interacting or merging system with two distinct components. The larger component exhibits a somewhat irregular morphology, displaying a central, bright region with a diffuse, extended halo. The color of the core is bluish-white, transitioning to a more teal color in the outer regions. This potentially indicates ongoing star formation within the core and a distribution of older stellar populations in the surrounding halo.

The second, smaller component is located nearby and shows a more compact, rounded morphology. It also possesses a central region that is bright with a bluish-white color.

There seems to be a disturbance in both galaxies' shapes suggesting this is an interaction/merger, with tidal forces potentially playing a role. There appears to be a faint bridge of material between the two galaxies. There does not seem to be significant dust obscuration present.
