The galaxy presents as a disk galaxy with a central bulge. The disk is not perfectly edge-on, but is significantly inclined to our line of sight. There appears to be a bar-like structure traversing the central region of the galaxy, though it is not sharply defined. Hints of spiral arms are visible, though not clearly delineated. The bulge exhibits a moderate size relative to the overall galaxy dimensions. There is no obvious evidence of ongoing major mergers, though subtle disturbances in the disk structure cannot be ruled out. Overall, the galaxy appears to be a relatively normal spiral galaxy.
