The galaxy presents as a disk galaxy, observed at a significant angle relative to face-on, displaying a moderate degree of flattening. The central region is characterized by a bright, concentrated bulge. The color of this bulge appears predominantly yellow to red, suggesting an older stellar population. Moving outward from the center, the galaxy exhibits a disk component. The color of the disk shifts towards a bluer hue, indicating the presence of younger, hotter stars and potentially ongoing star formation regions. The overall structure suggests a relatively undisturbed morphology, without any pronounced tidal features or signs of recent major mergers. There may be a spiral structure but it is difficult to identify. There is very little dust apparent in the image. 
