The galaxy presents a disk-like morphology, viewed at a high inclination, approaching edge-on. The central bulge appears moderately prominent, exhibiting a bright, yellowish hue, likely indicative of an older stellar population. Two spiral arms are suggested, though not clearly defined, possibly due to the galaxy's inclination. The arms are tightly wound in sections, with regions of medium winding, exhibiting a bluer color compared to the bulge, suggesting ongoing star formation. There is no obvious major merger, though the galaxy is surrounded by potential minor disturbances. No bar structure is visible.
