The galaxy presents as a disk-shaped structure viewed at an oblique angle, approaching edge-on orientation. There is evidence of a central bulge, appearing yellow-white in color, suggesting an older stellar population. The disk is visible, with a bluer hue than the central bulge, potentially indicative of ongoing star formation. Although the disk is truncated by the viewing angle, there are hints of spiral arm structures. There is no obvious major merger event apparent. The galaxy exhibits a moderate level of disturbance but appears relatively isolated. Overall, it appears to be a moderate-sized spiral galaxy with ongoing star formation.
