The observed galaxy presents a distinct spiral structure. Two prominent spiral arms emanate from a central bulge region. The arms appear somewhat loosely wound, extending outwards. The central bulge exhibits a moderate size relative to the overall galactic disk. A bar-like structure appears to be present in the central region. Evidence suggests the galaxy is undergoing some form of interaction, indicating a disturbed morphology, potentially due to minor gravitational influences. The primary colorations include a yellow-red core, potentially indicative of an older stellar population, transitioning into bluer hues within the spiral arms, which may denote ongoing star formation regions. There is no apparent edge on disc, but the disc itself has prominent features.