The galaxy appears to be a relatively well-defined, intermediate-sized system. It exhibits a central, bright bulge region, with a more diffuse and extended disk component surrounding it. The morphology seems to lean towards a spiral-like structure, although the arms are not clearly defined in the image. There is a degree of irregularity in the outer regions of the disk, suggesting possible minor interactions or disturbances. The galaxy displays a color gradient, with a yellowish-white hue dominating the central bulge, transitioning to a bluer color in the disk region. This implies the presence of older stellar populations in the bulge and younger, hotter stars within the disk. Overall, the galaxy appears to be in a relatively stable, evolved state.
