The observed galaxy presents as a spiral type with a moderate-sized bulge and a well-defined disk structure. A complex network of spiral arms originates from the central region, exhibiting a tightly wound morphology. There appear to be two distinct spiral arms emerging from the central bulge. The arms are relatively smooth in appearance with a moderate luminosity, and they span a considerable portion of the disk. The galaxy's light distribution suggests a redder core, transitioning to bluer hues towards the outer regions, indicative of younger stellar populations in the spiral arms. There appears to be a minor disturbance in the outer portion of the arm structure on one side of the galaxy, perhaps indicating a minor interaction. Overall, the system appears to be a relatively quiescent spiral galaxy, with well-formed arms and an ordered disk.
