The galaxy presents as a relatively smooth, elliptical-like structure. There is a concentration of light toward the center, suggesting a defined nucleus or core region. The overall shape appears somewhat elongated, but not strongly so, exhibiting a subtle departure from perfect circularity. No distinct spiral arms or other prominent features such as dust lanes are readily discernible. The color is generally whitish, with a slight bluish tinge in the central region, potentially indicating a component of younger, hotter stars, though the dominant stellar population appears evolved. There appears to be a very slight disturbance in the shape of the galaxy but is not obvious. No other interacting galaxies are visible in close proximity.
