The galaxy presents as a spiral structure with well-defined arms. The spiral arms exhibit a clumpy morphology, suggestive of ongoing star formation regions. The central bulge appears relatively moderate in size and luminosity. The disk is viewed at a noticeable angle, but not fully edge-on, allowing some of the spiral structure to be visible. There is a subtle indication of a bar-like structure spanning the center of the galaxy. The color distribution implies a relatively blue disk, with younger stellar populations compared to the bulge, which exhibits a more yellowish hue. The galaxy appears relatively isolated, with no immediately apparent signs of major interaction or ongoing merger activity, although some minor disturbances cannot be ruled out at this resolution.
