The galaxy presents a somewhat disturbed morphology, appearing to undergo a significant interaction or merger. There are faint, diffuse structures that extend outward, likely tidal tails indicative of gravitational disruption. The central region exhibits a bright, yellowish hue. The disk appears somewhat inclined to our line of sight, with hints of a spiral structure visible. There is an irregular distribution of light within the disk, with some patches or clumps of brighter regions, suggesting ongoing star formation or remnants of the merger event. The galaxy displays a color gradient, with a bluer tint in some of the outer regions, potentially indicating younger stellar populations. A moderately-sized bulge can be estimated from the structure.
