The galaxy presents as a spiral type, viewed at a slight angle relative to face-on, but not quite edge-on.  A distinct central bulge is visible, appearing yellow, possibly indicating an older stellar population concentrated in the core.  Two prominent spiral arms emanate from the central region. These arms appear relatively tightly wound. There's also the suggestion of fainter and more diffuse spiral structure extending further out from the main arms. The spiral arms exhibit a bluer hue compared to the central bulge, suggesting the presence of younger, hotter stars and ongoing star formation within the arms.  Overall, the galaxy appears to be relatively undisturbed, without obvious signs of a major merger or strong tidal interactions with other galaxies. There are subtle irregularities within the arm structure that could indicate minor interactions or internal dynamics at play. The disk appears to be very large compared to the size of the bulge.