The galaxy presents as an edge-on disk galaxy with a prominent bulge. Dust lanes are visible, obscuring the central region of the disk and adding to the reddish color. The bulge appears relatively large and concentrated, displaying a yellowish-orange hue, suggestive of an older stellar population. The disk component of the galaxy exhibits a bluer color, indicating the presence of younger stars and ongoing star formation. The overall color suggests a mix of stellar populations within the galaxy, with some signs of low levels of ongoing star formation. The disk exhibits a smooth morphology, with no apparent strong spiral arm structure visible. There are no obvious signs of recent major mergers or tidal disturbances, although minor disturbances cannot be ruled out. The galaxy appears relatively isolated.
