The galaxy presents as a highly inclined disk galaxy, viewed nearly edge-on. The central bulge appears prominent and elongated along the major axis, exhibiting a smooth, rounded profile. The disk component is visible as a faint, extended structure on either side of the bulge. There is a slight indication of dust lane obscuration along the midplane of the disk, closer to the bulge. Weak star formation appears to be present, concentrated in several HII regions. There is no apparent evidence of strong tidal features or ongoing major merger activity. The galaxy's morphology suggests that it is a late-type spiral galaxy.