The galaxy presents as a relatively compact structure. It appears largely smooth with a somewhat elliptical shape and little to no indication of spiral arms. The central region exhibits a brighter concentration of light, possibly indicating a nucleus or bulge.

There appears to be a subtle color gradient from the center outwards, with the central regions appearing slightly more yellow/white, potentially indicating an older stellar population, while the outer regions show a faint bluish tint suggestive of younger, hotter stars.

There is slight asymmetry in the outer regions, which could indicate a minor gravitational disturbance or recent interaction. However, the overall morphology does not suggest a major merger event.
