The galaxy presents a slightly irregular morphology. It exhibits a central, bright, concentrated region, likely a bulge, with a yellow/orange hue. Extending from this core is a fainter, bluish, disk-like structure to the left. The right side appears smooth but exhibits a spiral structure. This structure may be indicative of past merger events, or possible interactions with another, unseen galaxy. There may be some ongoing star formation. Overall, the galaxy's form appears intermediate between elliptical and spiral classifications.
