This galaxy exhibits a generally smooth morphology with a flattened, disk-like structure. The central region appears brighter and more concentrated, indicating a possible bulge or active galactic nucleus. Surrounding the central area is a slightly more diffuse region with hints of spiral arm structure, but these are not clearly defined. The color distribution suggests a mix of stellar populations, with a bluer hue in the inner disk perhaps indicating younger stars, and more red in the surrounding regions. There is some irregularity in the outer regions of the disk, which is not perfectly smooth and exhibits some disturbances. Overall, the galaxy presents as a relatively well-formed, though potentially disturbed, disk galaxy.
