The galaxy presents an elongated, disk-like structure, oriented approximately horizontally in the image. A central bulge appears to be present, with a concentration of light suggesting a higher stellar density in this region. The color profile transitions from a yellowish-white core outwards to a bluish hue on the outer edges. This suggests a difference in stellar populations, with older, redder stars concentrated in the core and younger, bluer stars distributed within the disk. The overall morphology seems relatively undisturbed, lacking obvious signs of recent major mergers or tidal interactions. There's a slight irregularity in the light distribution on one edge of the disk, potentially indicating a minor disturbance or the presence of spiral arm segments. Star formation seems to be ongoing, as evidenced by the blue color in the disk, but likely at a moderate rate given the overall color balance. The galaxy is of intermediate size and mass, with a well-defined disk structure and a centrally concentrated bulge.
