The galaxy presents a generally smooth and rounded morphology. Its color profile suggests an older stellar population, exhibiting a yellowish-orange hue. The light distribution is concentrated towards the center, indicating a prominent bulge or core region. While the main body appears relatively undisturbed, a faint, smaller object is visible in close proximity, potentially indicating a minor interaction or a satellite galaxy. There is no clear evidence of spiral arms or significant disk-like structures. The galaxy likely has a high stellar mass and a low star formation rate.
