The galaxy presents as an elongated, edge-on disk system. A prominent central bulge dominates the galaxy's core, displaying a yellowish-orange hue, suggesting a population of older, redder stars. The disk component, viewed nearly edge-on, exhibits a bluer color profile, indicative of younger stellar populations and ongoing star formation. The disk appears relatively smooth, without significant signs of spiral arm structure. There is minimal evidence of dust lanes within the disk. The galaxy appears to be undisturbed, without obvious signs of tidal interactions or recent merger activity. The bulge is round. Overall, it is a classic example of an edge-on disk galaxy with a significant bulge component.
