The galaxy appears to be a relatively smooth, elliptical-type galaxy. Its color profile suggests an older stellar population, with a yellowish-orange hue dominating its core. There is evidence of possible tidal interactions or minor disturbances in the galaxy's morphology. Faint extensions or irregularities are visible on one side of the object. The object exhibits a compact form, with a generally round or slightly oval shape, but these possible disturbances create a shape that deviates slightly from the standard elliptical form. The overall appearance suggests a system that is either in the late stages of a merger event, or may have undergone such an event in the past, which could account for the deviation in the shape. There is potentially some on going star formation within the core, but the overall star formation rate is low.
