The galaxy presents as a spiral type, exhibiting a distinct disk structure. Prominent spiral arms are visible, tightly wound around a moderately sized central bulge. The spiral arm morphology suggests the presence of multiple arms, possibly up to four, though resolution limits precise counting. A bar feature appears to be either weak or non-existent. The galactic disk shows a slight inclination, not quite edge-on. There is no obvious evidence of major mergers or significant tidal disturbances. The overall color profile indicates active star formation occurring within the spiral arms. The central bulge appears yellowish, possibly indicating an older stellar population.
