The galaxy appears to be a luminous, yellowish-white, elliptical-like structure. Its light profile appears mostly smooth, with no obvious spiral arms or bar structure visible. The morphology is primarily smooth, although there seems to be a slight asymmetry in the isophotes that may indicate a minor interaction or disturbance. The galaxy's color is relatively uniform, indicating a generally old stellar population, though the slight color gradient may suggest some ongoing, low-level star formation. The galaxy has a centrally concentrated structure and a relatively round shape. There's a possibility of interaction based on the disturbance, or perhaps it is an early stage merger with another object.