The galaxy presents as a relatively small, elongated structure, suggestive of a disk-like morphology viewed at a significant inclination. The central region exhibits a brighter, more concentrated luminosity profile, transitioning smoothly outward. A subtle colour gradient is observed, with the core appearing slightly yellower than the bluer outer regions. The overall structure appears largely undisturbed, displaying only minor irregularities in its shape. There are no obvious signs of intense star formation regions within the disk.
