The galaxy presents as an elongated, disk-shaped object seen nearly edge-on. A central bulge appears prominent, exhibiting a slightly reddish hue, potentially indicative of an older stellar population. Fainter, bluish-white light is observed emanating from the extended disk, possibly suggestive of ongoing or recent star formation activity. The disk seems relatively smooth, lacking prominent spiral arm structures. The galaxy displays a degree of asymmetry in its outer regions, hinting at potential interactions or tidal disturbances, though these features are not pronounced. Overall, the galaxy appears to be a relatively massive system undergoing moderate star formation.
