The galaxy presents as a spiral galaxy, observed at an angle between face-on and edge-on. The central bulge appears prominent, exhibiting a yellow-orange hue, suggesting an older stellar population. Spiral arms are faintly visible, extending from the bulge, and appear to be more loosely wound. These arms display a bluer tint, indicating the presence of younger, hotter stars and ongoing star formation, though it does not appear extremely active in this instance. The disk shows a slight asymmetry. Overall, the galaxy seems to be relatively undisturbed, showing no obvious signs of a major merger or strong tidal interactions.
