The galaxy presents as a spiral type, exhibiting distinct spiral arm structures originating from a central bulge. The spiral arms appear relatively tightly wound. Two dominant arms are discernable. The central bulge appears prominent, exhibiting a concentrated luminosity gradient towards the center. The overall color suggests a population of both older and younger stars, as indicated by the presence of both yellowish-red hues in the bulge and bluer colors in the spiral arms. Evidence of moderate star formation is implied by the colors of the spiral arms. There is no obvious indication of tidal tails or dramatic distortions suggesting a major merger. The image suggests a relatively undisturbed morphology.
