The galaxy presents as a spiral type, exhibiting a prominent disk structure. The spiral arms are tightly wound and relatively well-defined, although some degree of blurring and faintness makes precise tracing difficult. There appear to be two main spiral arms. There is a central bulge that occupies approximately one quarter of the galaxy's diameter. The galaxy's color appears to be yellow-green, suggesting an intermediate population of stars. The disk appears to be inclined relative to our line of sight, with an apparent ellipticity. Evidence for a bar structure is tentative but cannot be completely ruled out. The overall morphology suggests no significant recent merger events or major disturbances.
