This galaxy exhibits a disk-like structure, although it is not perfectly symmetrical. The disk is oriented at an oblique angle to our line of sight, presenting a somewhat tilted view. The central region displays a brighter, more concentrated luminosity, possibly indicating the presence of a bulge.  The spiral arms appear somewhat disrupted, with noticeable irregularities in their shape and distribution of light. There is evidence of significant disturbance throughout the disk, suggesting a possible ongoing or recent merger event. Patches of bluer light are distributed throughout the disk, which may indicate regions of active star formation.  A significant portion of the galaxy shows a relatively smooth distribution of light with a relatively smooth overall morphology, but the irregularities within the spiral arms and disk are still notable.
