The galaxy presents a spiral morphology, with a prominent central bulge surrounded by a disk. Spiral arms are distinctly observed, with two arms being the most prominent. These arms are moderately wound, not tightly coiled but not widely spread either. The bulge appears substantial in size, contributing significantly to the overall luminosity of the galaxy. There are indications of a bar-like structure within the central region, but it does not seem heavily pronounced. In addition, there may be some signs of disturbance or interaction, but it is subtle.
