The galaxy appears to be a spiral galaxy, viewed at a slight angle relative to face-on. Two prominent spiral arms are visible, tracing a well-defined pattern. The arms exhibit moderate winding, neither tightly wrapped nor loosely extended. The central bulge appears relatively small compared to the disk. There is some indication of a bar-like structure within the central region. No major disturbances indicative of a significant merger event are readily apparent, although minor irregularities in the arm structure cannot be ruled out. The disk dominates the light profile. The overall color suggests a mix of stellar populations, with bluer regions in the arms possibly indicating ongoing star formation and a slightly redder bulge indicative of older stellar populations.
