The galaxy presents as a spiral type, viewed at an oblique angle relative to our line of sight. The disk exhibits a prominent central bulge, though it does not visually dominate the overall structure. Faint spiral arms are discernible, appearing somewhat loosely wound and with two or more arms. There may be a weak bar-like structure within the central region. The galaxy appears relatively undisturbed, with no immediately obvious signs of major merging activity, although some minor irregularities could indicate a possible interaction. Color gradients suggest active star formation, particularly within the spiral arms. The overall morphology indicates a galaxy with a well-defined disk structure and an intermediate-sized bulge.