The galaxy presents as a disk-shaped structure, viewed at an oblique angle, with a noticeable central bulge. There is a bar structure crossing the galactic center, which appears relatively strong. Some spiral arm features are visible. The galaxy appears to be in a relatively relaxed state, with only minor disturbances. The overall color suggests a mix of stellar populations, with a slightly bluer hue in the disk, consistent with ongoing star formation. The central bulge shows a more yellow/orange color, suggesting an older stellar population.
