The galaxy presents as a disk-shaped structure, inclined at a significant angle relative to our line of sight. A central bulge is visible, exhibiting a yellowish hue, suggesting an older stellar population within the galactic core. The disk component displays a bluer color, indicative of ongoing star formation. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. Patches of relatively low luminosity appear throughout the galaxy.
