The galaxy presents as a relatively faint, elongated structure with a high degree of inclination, appearing nearly edge-on from our vantage point. The central region exhibits a concentration of light with a yellowish-orange hue, suggesting the presence of older stellar populations. Moving outward from the core, the color transitions to a bluer tint, indicative of younger, hotter stars populating the galactic disk. There is no discernable spiral structure due to the viewing angle. The galaxy appears largely undisturbed, displaying a symmetrical profile with no significant signs of tidal interactions or recent mergers. The bulge is subtle, without any boxy or unusually rounded characteristics evident. A faint, diffuse halo seems to surround the main disk, subtly extending the overall dimensions of the galaxy.
