The galaxy appears to be a spiral galaxy, exhibiting a distinct disk-like structure. There is a central bulge with a yellow hue, suggesting the presence of older stellar populations. Faint spiral arms are visible, extending from the bulge into the outer regions of the disk. These arms have hints of blue, suggesting the presence of younger, hotter stars, which implies some level of ongoing star formation activity within the disk. The galaxy's disk is tilted relative to our line of sight. The overall shape of the galaxy is elongated, with a relatively smooth texture. There is no indication of any major mergers or significant tidal disturbances based on this single image.
