The galaxy presents as a relatively faint, elongated object, indicative of a disk galaxy viewed at a high inclination, nearly edge-on. There is a noticeable central bulge which appears smooth and concentrated, potentially suggesting an older stellar population. The disk component shows evidence of structure, possibly spiral arms, though these are tightly wound and not clearly resolved. The color gradient across the galaxy suggests that the central bulge exhibits a yellowish hue, while the outer disk shows hints of bluer colors. This could indicate ongoing star formation in the disk and a more quiescent stellar population in the bulge. There may be some minor disturbances visible within the disk, such as faint tidal features, that are subtle. The galaxy appears to not be undergoing significant star formation and has a stellar mass around 10^9 solar masses. There are no signs of a major merger event.
