The galaxy presents as an elongated, disk-like structure with a relatively smooth overall appearance. The central region exhibits a brighter concentration of light, suggesting a nucleus or bulge. The color profile indicates a blueish hue in the central part of the galaxy, with a gradual shift towards redder tones in the outer regions of the disk. There are subtle indications of possible disturbances or minor irregularities in the disk's morphology, hinting at potential interactions or internal dynamical processes. The overall shape leans towards an intermediate elliptical nature.
