The galaxy presents a somewhat inclined disk morphology, with a notable central bulge. The bulge appears to be of moderate size relative to the overall disk. Spiral arms are visible, exhibiting a loosely wound structure. Two dominant spiral arms are observed, with possible additional fainter arms. The galaxy exhibits a distinct bar feature that extends through a significant portion of the galaxy. The galaxy may be undergoing minor interactions or disturbances as subtle asymmetries can be seen. The disk is not perfectly smooth. The galaxy appears to be relatively large.