The galaxy presents as a disk-shaped system, with a noticeable bulge. The bulge region is brighter and has a yellowish hue, suggesting an older stellar population. Extending outwards from the bulge is the galactic disk, exhibiting a bluer color, indicative of ongoing star formation and a younger stellar population. The outer regions of the disk appear fainter and less defined, possibly due to lower stellar density or obscuration by dust. The overall shape is elongated, suggesting an elliptical morphology. The disk appears to be inclined relative to our line of sight. There is no clear evidence of spiral arm structure. There are faint features and patches of light with slightly varying hues on the edges of the disk, but the galaxy is mostly smooth.
