The galaxy presents as a slightly elongated, disk-like structure, though appearing largely smooth and featureless. The central region exhibits a concentrated luminosity, suggesting a prominent galactic bulge or core. There is a noticeable color gradient from the center outwards, with the core displaying a yellowish-orange hue, transitioning to a bluer tint in the outer regions, potentially indicative of younger stellar populations. The overall structure shows only minor disturbances, with a high probability of no merging events significantly impacting its form. The galaxy displays moderate star formation activity, supported by the presence of the bluer regions. The estimated size suggests a substantial physical extent, likely exceeding the typical dimensions of smaller galaxies, but still within reasonable bounds. The disk is tilted relative to our line of sight, giving it an elliptical appearance in the image.
