The galaxy presents as an elongated, disk-shaped structure, viewed nearly edge-on. A prominent central bulge is visible, exhibiting a concentration of light suggesting a higher density of older stellar populations. The bulge appears smooth and spheroidal in shape. The disk component displays a relatively homogenous color distribution. Faint hints of dust lanes are possibly present along the galactic plane, though image resolution limits definitive confirmation. There are no indications of major disturbances, tidal tails, or other features indicative of a recent major merger. The galaxy exhibits an overall smooth morphology.
