The galaxy exhibits a distinct spiral structure, with well-defined arms emanating from a central bulge. These arms show a winding pattern that appears to be primarily of medium tightness, with some loose aspects. Patches of bluer light are visible along the arms. The central bulge appears of moderate size, though not completely dominant. There's some evidence of disturbance in the galaxy's overall structure, potentially indicating minor interactions or mergers. The galaxy is not seen edge-on. Bar structures, when present, do not seem strongly defined. The color gradients suggest active star formation regions within the spiral arms. The shape is not perfectly symmetrical, hinting at ongoing dynamic processes within the galaxy or external influences.