The galaxy presents as an elongated structure, viewed nearly edge-on. A prominent, centrally located bulge is observed, exhibiting a yellowish-orange hue, suggestive of an older stellar population. The bulge appears relatively smooth and rounded. A disk component is evident, extending outwards from the bulge. The disk is significantly fainter and bluer in color compared to the bulge, implying ongoing star formation. The disk is highly inclined with respect to our line of sight. Possible tidal disturbances or minor interactions may be subtly perturbing the disk's morphology, evidenced by a faint, blue, arm like structure extending from one end. No signs of a major merger are apparent.
