The observed galaxy presents as a roughly elliptical, disk-shaped structure. A central bulge is discernable with a high surface brightness, appearing nearly uniform in color. The disk component appears complex, with faint spiral arm segments or tidal features emanating away from the central bulge. The galaxy’s overall color appears relatively blue, suggesting a population of younger, hotter stars and ongoing star formation, particularly in the disk regions. There is a noticeable asymmetry to the disk, with one side appearing more extended and diffuse than the other. A faint linear feature extends from the primary disk. This feature, based on its geometry and lower surface brightness, is potentially a tidal tail. Overall, the morphology suggests a system experiencing some form of interaction or disturbance, but not a clear, ongoing major merger.
