The galaxy appears to be a spiral type, exhibiting a disk-like structure with prominent spiral arms. The spiral arms are loosely wound, extending outward from the central bulge. Two arms appear to be dominant. The central bulge appears moderately sized, with a yellowish hue, suggesting an older stellar population. The arms exhibit a bluer color, indicating the presence of younger, hotter stars and ongoing star formation. There is no obvious indication of a strong bar feature bisecting the bulge. There are suggestions of minor disturbances in the morphology, but no large merger activity or obvious tidal tails are visible. The galaxy is not viewed edge-on, allowing us to see the spiral arm structure.
