The galaxy appears to be a spiral galaxy, viewed at a considerable angle away from face-on. Prominent spiral arms are visible, with a relatively tightly wound structure. The arms exhibit a clumpy morphology, likely indicating regions of active star formation. A noticeable central bulge is present, with an elongated, bar-like structure possibly bisecting the core region. The bar appears to be a weak bar. There is no apparent dominant bulge, but the central bulge is a clear and defined portion of the galaxy. The overall color of the galaxy is generally blue, with a concentration of redder hues toward the central regions, potentially indicating a difference in stellar populations. There are no obvious signs of a recent major merger, though some minor tidal features or asymmetries cannot be ruled out based on the image alone. A slight distortion in the galaxy's outer spiral arms may indicate some gravitational interaction. The galaxy does not appear to be a completely smooth elliptical, and shows no significant indication of being an artifact.