The galaxy presents as a relatively smooth, disk-like structure viewed at an oblique angle. Its central region exhibits a concentrated, bright luminosity suggesting a significant stellar population. The color gradient indicates an older stellar population dominating the bulge, shifting toward bluer hues in the outer regions of the disk, implying ongoing star formation in those areas.

There is a suggestion of a minor disturbance, potentially a faint tidal feature or a small companion galaxy interacting with the primary galaxy.
