The galaxy presents a somewhat diffuse appearance, with a suggestion of spiral structure, though the arms are not well-defined. The central region appears brighter, indicating a possible bulge, although it does not dominate the overall structure. The disk of the galaxy seems to be inclined relative to our line of sight, hinting that we are not viewing it face-on. There is evidence of ongoing or recent interaction or merging activity, with significant disturbance to its morphology. Patches of bluer light may indicate regions of more recent star formation. No prominent bar structure is visible.
