The galaxy presents as a spiral type with a prominent central bulge, displaying a yellowish hue suggesting an older stellar population. The galaxy is viewed at an angle, not quite edge-on but significantly inclined, obscuring a full view of the disk. The spiral arms are tightly wound and appear distinct, extending from the central region, although precise arm count is difficult to ascertain due to the inclination. There is a moderate amount of dust obscuration apparent within the arms. The galaxy appears relatively isolated, exhibiting no immediate signs of major mergers or tidal disturbances. The outer disk fades gradually, indicating a smooth decline in stellar density from the center outwards. There may be a weak bar structure present, but this is difficult to confirm given the galaxy's orientation.
