The galaxy presents a complex morphology, appearing as a relatively compact structure with an estimated effective radius of a few kiloparsecs. The central region is dominated by a bright, yellowish component, indicative of an older stellar population. The galaxy exhibits faint spiral arm features that extend outward from the core, although these are somewhat ill-defined and patchy, suggesting a disturbed or flocculent spiral structure. There is a faint, diffuse halo surrounding the main body of the galaxy. Overall, the morphology is ambiguous. The low star formation rate suggests that star formation activity within the galaxy is currently suppressed.
