This galaxy appears to be a spiral galaxy, exhibiting a relatively small bulge and a prominent disk structure. The spiral arms are well-defined and display a loose winding pattern, extending outwards from the central region. Two dominant spiral arms appear to be present. There is evidence of a bar-like structure spanning across the galactic center, the bar seems moderate. The disk appears slightly inclined with respect to our line of sight. There are no obvious signs of ongoing major merging events, although a slight asymmetry in the outer disk may suggest a minor interaction or disturbance. Patches of blue light are observed within the spiral arms, likely indicating regions of active star formation.
