This galaxy presents as a somewhat elongated, disk-shaped structure viewed at a significant angle, likely approaching edge-on. The central region exhibits a bright, concentrated luminosity indicative of a bulge, which could be composed of older stellar populations. Moving outwards from the central bulge, the galactic disk shows a bluer hue, possibly suggesting ongoing star formation in this region. The edges of the galaxy appear somewhat indistinct, displaying no clear, sharp boundaries, which may suggest a degree of tidal interaction or a more diffuse distribution of outer stellar populations. The overall appearance is relatively smooth, although subtle variations in color and brightness are discernible across the galactic structure. No prominent spiral arm structures are visible, but the galaxy has features and disks.
