This galaxy presents as a thin, elongated disk, viewed nearly edge-on. The central bulge appears prominent and spheroidal, exhibiting a yellowish-orange hue, suggesting an older stellar population. The disk is more elongated than the bulge, with a slight inclination relative to our line of sight. 

The disk shows a subtle color gradient, with the regions closer to the bulge displaying a similar yellow-orange coloration, transitioning to slightly bluer tones at the outer edges. This bluer coloration might indicate regions of active star formation. Dust lanes are not clearly discernible, however, there are slight irregularities within the disk's brightness, indicating the presence of obscuring material. There is no evidence of recent major merger activity, however, there could be minor disturbances in the disk, as the galaxy is not perfectly symmetrical and the light distribution shows some faint asymmetries. The overall morphology suggests a relatively undisturbed spiral galaxy, with a large disk and prominent bulge.
