The galaxy presents as a flattened, disk-like structure viewed at an oblique angle. The central region exhibits a high surface brightness, appearing nearly unresolved and intensely luminous in the image. Moving outwards from the core, the surface brightness decreases, with the disk exhibiting a mottled texture, which could be indicative of spiral arm structures or irregular dust lanes. The overall color profile shows a slightly bluer hue in the outer regions of the disk compared to the central bulge, potentially suggesting a higher proportion of younger, hotter stars in the periphery. The galaxy also appears to have an irregular morphology, where the shape deviates from a perfect ellipse, possibly indicating a gravitational interaction with another galaxy.