The galaxy exhibits a prominent central bulge that appears yellowish-white, suggesting an older stellar population. Surrounding the bulge is a fainter, more diffuse disk. The disk presents with a bluish hue, indicative of younger, hotter stars and ongoing star formation. There is a slight indication of spiral arm structure, but the disk appears relatively smooth overall. The galaxy's inclination suggests it is viewed at a moderately oblique angle. There is a hint of possible tidal distortion or minor disturbance in the outer regions of the disk, with the overall shape departing slightly from a perfect elliptical symmetry.
