The galaxy appears as a relatively small, elongated object with a smooth, elliptical morphology. It exhibits a central concentration of light that gradually diminishes towards its outer edges. The core region displays a reddish hue, potentially indicating an older stellar population. The outer regions of the galaxy appear bluer in comparison, suggesting the presence of younger stars or active star formation. Some subtle irregularities or faint extensions are possibly present in the galaxy's outskirts. No strong spiral arm features or a distinct galactic disk can be clearly identified. There are possible signs of a minor disturbance. 
