The galaxy presents an overall smooth morphology with a distinct, elongated shape, suggesting it is viewed nearly edge-on. There is little evidence of spiral arms or significant dust lanes. The central region of the galaxy appears brighter and has a yellowish-orange hue, which could indicate an older stellar population. The outer regions exhibit a bluer tinge, possibly suggesting more recent star formation activity. The galaxy's light appears fairly uniform, with no obvious signs of significant starburst regions or active galactic nucleus. There appears to be no major ongoing mergers or tidal disturbances visible, with no nearby companions that would be indicative of an interaction. Overall the galaxy seems to be a relatively undisturbed system.
