The galaxy presents a clear, elongated, disk-like structure, strongly suggesting an edge-on or nearly edge-on orientation relative to our line of sight. A prominent central bulge is visible, exhibiting a yellowish-white hue that likely indicates an older stellar population. The disk itself displays a reddish-orange coloration, possibly indicating a dusty environment with ongoing or recent star formation. There is a degree of smoothness to the overall light distribution, suggesting a lack of significant recent mergers or major disturbances. The dust may be obscuring some details in the disc. Overall, this galaxy appears to be a fairly quiescent system.
