The galaxy presents as a spiral galaxy, inclined relative to our line of sight. It exhibits a moderate-sized bulge, with tightly wound spiral arms extending outwards. The bulge is notably brighter and more yellow in color compared to the disk, suggesting an older stellar population. The spiral arms show a clumpy structure, indicative of ongoing star formation regions. A prominent bar structure is visible, spanning a significant portion of the galaxy's central region. There is no evidence of a major ongoing merger, but some minor disturbances cannot be ruled out. Overall, it presents as a barred spiral galaxy with evidence of both an aging bulge population and active star formation within its spiral arms.
