The galaxy presents a morphology consistent with a barred spiral galaxy, exhibiting a prominent central bar structure. Two distinct spiral arms emanate from the ends of the bar, displaying a relatively well-defined structure. The winding of the spiral arms appears to be intermediate, neither tightly wound nor excessively loose. The central bulge is visible but not dominant, appearing as a moderate to small component of the overall galactic structure. The overall color suggests ongoing star formation, as indicated by the presence of bluer regions within the spiral arms, contrasting with the yellower hue of the central bulge. There is no obvious evidence of major mergers or significant tidal disturbances, though minor asymmetries in the outer arms cannot be ruled out with certainty.
