The galaxy presents as a moderately luminous, elliptical-like structure, exhibiting a smooth, centrally concentrated morphology. It appears largely featureless. The color profile suggests an older stellar population, with a yellowish-red hue dominating the central bulge. There is no indication of prominent spiral arms or significant dust lanes. The overall shape is somewhat elongated, but not highly distorted, implying a relatively relaxed and stable system. There are no apparent signs of a major ongoing merger, though some minor disturbance or interaction is not entirely ruled out based on slight asymmetries in the outer regions of the galaxy.
