The galaxy presents as an elongated, somewhat spindle-shaped structure. It is observed at an oblique angle, suggesting it is likely a spiral or lenticular galaxy seen nearly edge-on. The central region exhibits a brighter, more concentrated luminosity, possibly indicative of a bulge or core. Moving outward from the center, the light becomes more diffuse and slightly bluer in hue, potentially suggesting the presence of spiral arms or a disk with ongoing star formation. The overall smoothness of the galaxy suggests it is relatively undisturbed, although some subtle irregularities may be present within the disk. There's a faint, elongated structure hinting at a possible dust lane or subtle warp within the galaxy's plane. The galaxy does not appear to be undergoing any major mergers or interactions with other galaxies.
