The galaxy presents a morphology that suggests a possible interaction or merging event with another galaxy or object. One component appears as a relatively smooth, elliptical-like structure, with a concentrated core and a diffuse halo. Its color profile indicates an older stellar population, based on its redder hue. Adjacent to it is a second, more compact, brighter component. This component exhibits a more pronounced orange-yellow color, possibly indicating ongoing or recent star formation. 

The overall morphology appears to be disturbed, which supports the possibility of an interaction. The relative proximity of the two components also suggests they are gravitationally bound, though further spectroscopic analysis would be needed to confirm.
