The galaxy appears to be a spiral galaxy viewed at a relatively high inclination, though not perfectly edge-on. The central bulge appears moderate in size and exhibits a yellowish hue, suggesting an older stellar population. Faint spiral arms are visible emanating from the central bulge, displaying a tightly wound morphology. The arms show hints of blue color, which could be indicative of on-going star formation regions. There is no strong evidence of a bar structure within the central region. The disk component appears relatively undisturbed, without major signs of tidal disruption or ongoing mergers. The galaxy exhibits a smooth, relatively symmetric structure.