The galaxy appears to be a spiral galaxy, oriented nearly edge-on to our line of sight. There is evidence of a prominent central bulge. Significant dust obscuration is likely present within the galactic disk, potentially influencing the observed color gradients. A possible tidal feature is observable, extending outwards, suggesting a potential gravitational interaction or merger event in the past. A close companion could be influencing its morphology. The disk exhibits a moderately blue color, indicative of some ongoing star formation.
