The galaxy presents a primarily disk-like structure, though its orientation relative to our line of sight obscures a clear view of any potential spiral arm morphology. There is some evidence for loosely defined and flocculent spiral structures. A central bulge component appears prominent, exhibiting a smooth, concentrated luminosity profile, transitioning into the fainter disk. The outer regions of the disk display some degree of irregularity. No strong bar-like structure is readily apparent within the central region of the galaxy. The overall color profile suggests a relatively mature stellar population dominating the bulge, while star formation activity, if present, appears subdued within the disk. There are no obvious signs of a major ongoing merger, although subtle distortions within the outer disk regions might suggest minor gravitational interactions.
