The galaxy presents as a primarily smooth structure, with a significant fraction of its light emanating from a rounded central region. It exhibits some characteristics indicative of possible merging activity. Although the primary shape is smooth, there appears to be some minor disturbance in its morphology. The galaxy shows a distinct color gradient, trending from more yellow-orange in the central region to a slightly bluer hue in the outer portions. The absolute magnitudes suggest this is a bright galaxy. Star formation is present within the galaxy.