This appears to be a spiral galaxy, viewed at an oblique angle relative to its disk. The central bulge is prominent, displaying a yellowish hue. The spiral arms are fairly well-defined, with a notable concentration of star formation regions exhibiting a bluish tint. The arms are wound moderately tightly around the bulge, with two dominant arms visible. There is a suggestion of a bar-like structure across the central region of the galaxy. Overall, the galaxy exhibits a moderate level of disturbance, potentially indicative of past minor interactions. The galaxy shows evidence of ongoing star formation.