The galaxy presents as a spiral type, with a moderately sized bulge. The spiral arms are prominent and well-defined, extending outwards from the central bulge. The arms exhibit a slightly flocculent structure, with some clumpy regions that are likely areas of active star formation. The disk of the galaxy appears inclined relative to our line of sight, but not edge-on. There is a faint indication of a bar structure spanning the central region, although it is not particularly strong. The bulge itself appears relatively smooth and bright, potentially indicating an older stellar population. There is no clear evidence of a major ongoing merger. The galaxy exhibits a moderate degree of blue color in its spiral arms, which hints at continuing star formation.