The observed galaxy presents as a moderately inclined spiral. Two prominent spiral arms can be distinguished. The central bulge appears subdued, its light gently fading into the disk. The disk exhibits a slightly flattened elliptical shape, with some obscuration possibly due to dust lanes. The winding of the spiral arms appear to be medium to loose. There is no obvious interaction or major disturbance with any other galactic body in the immediate vicinity. The overall color seems to be somewhat blue, suggesting ongoing star formation, particularly within the spiral arms.
