The galaxy presents as a slightly tilted disk galaxy, viewed at an oblique angle relative to its rotational axis. A prominent central bulge is apparent, exhibiting a yellowish hue indicative of an older stellar population. The disk component displays a mottled appearance with hints of spiral arm structures, though these are not sharply defined. The disk appears elongated along one axis, with a relatively high ellipticity. Fainter, diffuse extensions are visible at the periphery of the disk, potentially representing tidal features or the outer reaches of the galactic halo. Overall, the galaxy appears relatively undisturbed, lacking any obvious signs of major merger events, though a minor disturbance may be occurring.
