The galaxy presents as a relatively well-defined spiral galaxy, likely seen at a moderate inclination. The central bulge appears prominent and exhibits a reddish hue, suggesting an older stellar population. The spiral arms are somewhat tightly wound and demonstrate a bluish tint, indicative of ongoing star formation. There is a slight asymmetry observed within the spiral structure, potentially hinting at past minor interactions or internal disturbances. Overall, the galaxy appears to be a mature spiral galaxy.
