The galaxy presents as a flattened, disk-like structure seen nearly edge-on. Its light distribution suggests a smooth, centrally concentrated bulge, with a gradual decrease in luminosity towards the visible edges of the disk. The color profile indicates a slightly bluer hue, potentially indicative of ongoing star formation activity. The narrow width of the disk suggests a high inclination angle relative to our line of sight. No spiral arm structures or distinct dust lanes are clearly discernable in this image, implying a relatively uniform distribution of stellar populations and interstellar medium within the disk, or obscuration due to the edge-on viewing angle. The galaxy's overall morphology appears undisturbed, lacking evidence of any major mergers or tidal interactions.
