The galaxy presents an elongated, cigar-shaped morphology, with a smooth, somewhat diffuse structure. A central, brighter region suggests a nucleus or bulge. Proceeding outward from this central region, the light appears to transition into a bluer hue, which is suggestive of younger stellar populations. The overall smoothness indicates a relatively undisturbed system, without obvious signs of major mergers or tidal disruptions. It may have some form of ongoing, low-level star formation activity. The galaxy is likely viewed edge-on or at a high inclination.
