The galaxy appears to be a spiral galaxy exhibiting a disk-like structure. The disk shows a prominent bar feature crossing through its central region. Spiral arms emanate from the ends of this bar, displaying a relatively loose winding pattern. A moderate-sized bulge is visible at the galaxy's center, appearing as a concentrated region of increased brightness. The galaxy is not perfectly face-on; it is tilted somewhat with respect to our line of sight, presenting an elliptical appearance. The disk exhibits a clumpy morphology, likely due to the presence of star-forming regions. There do not appear to be any signs of ongoing major merging events.
