The galaxy presents as a flattened, disk-like structure with an elongated appearance. Its central region exhibits a bright, concentrated luminosity, suggesting a prominent galactic nucleus. Moving outward from the core, the brightness gradually diminishes into a fainter, more diffuse halo. The overall color profile indicates a mix of stellar populations. The central region appears relatively whiter, possibly indicating a higher concentration of older, less massive stars. Towards the outer regions, a subtle blue tint is observed, potentially suggesting the presence of younger, hotter stars and ongoing star formation. There is a slight warping of the disk morphology suggesting possible minor gravitational interactions. No spiral arm structures are readily discernible in the image.
