The galaxy presents a prominent disk structure, inclined relative to our line of sight. The disk exhibits spiral arm features, though the resolution limits a detailed tracing of their morphology. A notable central bulge is present, displaying a relatively high surface brightness compared to the disk. The spiral arms appear somewhat flocculent, with indications of both regions of active star formation and dust lanes. There is a potential bar-like structure in the central region. Overall, the galaxy exhibits a relatively smooth, undisturbed morphology.
