This galaxy presents as a relatively smooth, elliptical-like structure. Its central region displays a brighter, concentrated luminosity, suggestive of a substantial stellar population or perhaps an active galactic nucleus, though the resolution is insufficient to confirm the latter. Moving outward from the center, the galaxy exhibits a diffuse, less intense luminosity gradient. There is evidence of a faint, disk-like structure surrounding the central bulge, although its morphology is not sharply defined. The overall color is a muted bluish-white, hinting at the presence of a moderate amount of younger, hotter stars in addition to an older stellar population. There may be some minor disturbances in the galaxy's shape which indicates a possible interaction or merger in its past. The resolution does not permit detailed analysis of any spiral arm structures or individual star-forming regions.
