This galaxy presents as a barred spiral, although the bar is not sharply defined. The galactic disc is oriented at a moderately inclined angle relative to our line of sight. A prominent central bulge is visible, exhibiting a yellowish hue suggestive of an older stellar population. The spiral arms, while present, are not tightly wound, displaying a more open structure. These arms show evidence of ongoing star formation, indicated by the presence of bluer regions and clumpy structures. Overall, the galaxy appears to be a substantial system with a well-defined structure and active star formation within its spiral arms, and a bar that could be influencing this star formation. 
