The galaxy presents as a spiral type, seen at an inclined angle. It exhibits a distinct disk structure with prominent spiral arms. The arms are not tightly wound, displaying a more open morphology. There appear to be two dominant spiral arms originating from the central region. The central bulge appears moderate in size, exhibiting a yellowish hue, potentially indicating an older stellar population. The disk shows bluer regions within the spiral arms, indicative of ongoing star formation. The overall color suggests a mix of stellar populations, with both younger, bluer stars and older, redder stars present. There is no readily apparent sign of a major ongoing merger, although a minor disturbance may be present. A weak bar structure may exist within the central region.
