This galaxy presents a classic spiral morphology. Prominent spiral arms emanate from a bright, moderately sized central bulge. The spiral arms appear well-defined and exhibit a relatively tight winding pattern. A bar-like structure is present across the central region of the bulge. There is a slight asymmetry visible in the spiral arm structure, potentially indicating a minor gravitational interaction or disturbance. The overall color suggests active star formation, particularly within the spiral arms where bluer hues are observed. The galaxy's disk is not seen edge-on, but rather at a significant angle to our line of sight. There is no obvious sign of a major merger occurring within the galaxy.
