The galaxy presents as a generally smooth, elliptical structure. The central region exhibits a higher concentration of light, suggesting a prominent galactic nucleus or a dense stellar population. The overall color appears to be slightly blue-white, especially in the center, which could imply the presence of younger, hotter stars, possibly indicating some ongoing, albeit low, star formation activity. The morphology is somewhere between round and cigar-shaped. There are no obvious signs of major disturbances or ongoing mergers in the visible structure, although there is slight asymmetry in the outer region.
