The galaxy presents as a disk-shaped structure, viewed at a significant inclination. This near edge-on orientation complicates a clear assessment of its spiral arm structure. The central bulge appears prominent and concentrated, exhibiting a yellowish-orange hue suggesting an older stellar population. The disk component shows a color gradient, transitioning to bluer tones towards the outer edges, indicative of ongoing star formation. The galaxy lacks any obvious signs of major mergers or tidal disturbances, maintaining a relatively undisturbed morphology. Faint dust lanes are possibly present within the disk, though the image resolution limits definitive confirmation.
