This galaxy appears to be a spiral galaxy viewed at a moderate inclination, being neither quite edge-on nor face-on. A central bulge is visible, exhibiting a yellowish-orange color, suggestive of an older stellar population with relatively little ongoing star formation. Extending outwards from the bulge, faint spiral arms can be discerned. These arms display a bluer hue, which likely indicates the presence of younger, hotter stars and regions of active star formation. 

There seems to be some asymmetry present in the outer regions, possibly indicating some gravitational disturbance. The galaxy is moderately large, suggesting a substantial mass. Overall, the galaxy presents a mix of morphological features, hinting at a complex evolutionary history, including an actively forming disk with a more passive bulge.
