The galaxy presents as a smooth, elliptical-like structure. The central region exhibits a concentrated, bright core with a yellowish-orange hue. This color suggests an older stellar population dominating the core. Moving outwards from the center, the color shifts to a slightly bluer, less intense shade, implying the presence of younger stars, although the overall stellar population appears primarily aged. The galaxy's shape is elongated, indicating it is not perfectly spherical. No distinct spiral arms or significant dust lanes are visible. There is no clear evidence of a major ongoing merger, though the fuzzy edges could indicate minor tidal disturbances or interactions. The galaxy appears relatively isolated.
