The galaxy presents as an elongated structure with a well-defined central bulge. The core region exhibits a yellowish hue, suggesting a population of older stars, potentially dominated by red giants. Moving outward from the center, the galaxy fades in intensity, transitioning to a bluish-white color. The outer regions are diffuse and lack distinct spiral arm features, exhibiting a relatively smooth morphology. The overall shape appears flattened, hinting at a possible disk-like structure viewed at an angle. There are no obvious signs of major recent mergers or tidal disruptions in the immediate vicinity.
