The galaxy presents as a narrow, elongated, edge-on disc galaxy. Its central region appears slightly brighter, hinting at the possible presence of a bulge. The disc component exhibits a smooth texture with an apparent lack of distinct spiral arm structures. The galaxy's blueish hue suggests a relatively young stellar population with ongoing or recent star formation. There appears to be significant dust extinction obscuring the far end of the galaxy, as indicated by the lack of brightness. Overall, the galaxy appears relatively isolated and undisturbed, with no apparent signs of recent major mergers or tidal interactions.
