This galaxy exhibits a roughly elliptical morphology, though its shape deviates noticeably from a perfect ellipse. There appears to be some asymmetry, with the northern edge appearing somewhat more extended or disturbed than the southern edge.

The color distribution within the galaxy is not uniform. A central region appears bright and dominated by bluer wavelengths, potentially indicative of a population of younger, hotter stars or ongoing star formation. Progressing outward from the center, a green halo is observed. The outer regions show patches of redder light, which could be attributed to older stellar populations or dust obscuration. Some small regions of redder light are present more centrally.

Overall, the galaxy’s structure suggests possible ongoing or recent interactions. The slight distortions in shape, in combination with the color variations, suggest dynamic processes are at play. While not overtly displaying characteristics of a major merger, the irregularities might indicate a minor disturbance event.
