The galaxy presents as a somewhat tilted disk system, exhibiting a dominant central bulge that appears smooth and concentrated. The disk component is clearly visible, showing a slight asymmetry. There is an indication of spiral arm structure, appearing flocculent and not well-defined, with some blue hinting at on-going star formation within the disk. The overall color is yellowish-white, suggesting a relatively old stellar population, particularly within the bulge. The galaxy does not show strong evidence of a major ongoing merger, though some minor disturbances cannot be ruled out. The apparent edge-on orientation provides insight into the vertical structure of the disk and the prominence of the central bulge.
