The galaxy presents as a disk-shaped system viewed nearly edge-on. The central bulge appears bright and concentrated, exhibiting a yellowish-white hue, suggestive of an older stellar population. The disk itself is less defined, presenting as a fainter, bluer halo extending outwards from the bulge. The gradient suggests a smooth transition from the dense center to the sparser outer regions of the disk. No distinct spiral arm structures or dust lanes are readily apparent. The galaxy's overall morphology appears relatively undisturbed, showing no major signs of ongoing mergers or significant tidal disruptions. The shape is elongated, with a high ratio of major to minor axis, confirming its edge-on orientation.
