The galaxy appears to be a spiral galaxy with a prominent disk structure. The spiral arms are well-defined and loosely wound, extending outwards from a central bulge. The bulge is of moderate size, neither dominating the galaxy's structure nor being negligibly small. The galaxy is not seen edge-on; the disk is presented at an angle that allows us to discern the spiral structure. There is evidence of distinct regions of star formation within the spiral arms, characterized by a bluer hue. There appears to be no strong central bar structure, though a weak bar cannot be entirely ruled out based on visual inspection. No significant signs of ongoing major mergers or tidal disturbances are observed, although minor disturbances could be present. The galaxy exhibits a smooth but noticeable transition in color from the central bulge to the outer disk.
