The galaxy presents a somewhat inclined disk-like structure. Prominent spiral arms are visible, emanating from a central bulge region, which appears moderately sized. The arms show clumpy regions of star formation. A bar-like feature appears present, though not particularly strong, bisecting the central bulge. Overall, there are no indications of a major ongoing merger, although some signs of minor disturbance are visible in the outer disk. The galaxy exhibits a somewhat smooth overall appearance, yet featured, potentially from the spiral arms. Some dust lanes are possibly present but difficult to distinguish. The color gradient suggests active star formation regions.
