The galaxy presents as a system exhibiting evidence of interaction or merging activity. The primary component appears elliptical, possessing a diffuse, smooth morphology. The light profile suggests an older stellar population, with a yellow-red hue dominating the visual spectrum. A fainter component exhibits a bluer color, possibly indicative of ongoing star formation or a younger stellar population. There is also an indicator of minor structural disturbance in the main component, with some visible deformation. The overall shape of the interacting system is elongated, with some faint light extending from the edges of the two main components. The system's morphology suggests it is transitioning between stages in its evolution, potentially towards a more relaxed, elliptical form after the interaction is complete.
