The observed galaxy presents as a spiral type, characterized by a central bulge and prominent, well-defined spiral arms. The bulge appears relatively small and compact compared to the overall galactic disk. The spiral arms exhibit a distinct winding pattern that would be described as moderately wound. Two spiral arms appear to be dominant. There is indication of disturbances within the galaxy, showing some asymmetrical features, perhaps evidence of past or ongoing gravitational interaction. The overall color suggests a mix of stellar populations, with some bluer regions indicating recent star formation and yellower regions indicating older stars. There is a slight hint of a bar feature within the central region, although it is not prominently expressed. There does not appear to be an edge-on presentation.
