The galaxy presents a notable disk structure, characterized by prominent spiral arms. These arms are not tightly wound, suggesting an intermediate Hubble type. The arms exhibit a clumpy morphology, potentially indicative of ongoing star formation regions. A central bulge is visible, appearing moderately sized in relation to the disk. There is no apparent bar structure visible. There may be a minor tidal disturbance, but the galaxy overall seems relatively undisturbed with no indication of a significant merger event. The galaxy's color profile suggests a mix of stellar populations, with bluer regions along the spiral arms indicating younger, hotter stars, while the central bulge appears more yellow/red, indicating an older stellar population. The galaxy appears to have an inclination angle that makes it slightly edge on to our line of sight.