The galaxy presents as a relatively smooth, elliptical-like object with a concentrated central region. A slight elongation is observed, with the major axis oriented in a roughly northwest-southeast direction. The light distribution suggests a fairly uniform stellar population throughout the galaxy, with the highest density occurring in the core. Subtle color variations can be discerned, with the core appearing slightly whiter or bluer than the outer regions, which exhibit a more yellowish or reddish hue. The overall structure gives the impression of a galaxy with a well-mixed stellar population. There are no apparent signs of prominent spiral arms or significant dust lanes. Based on this, the galaxy is likely an elliptical or lenticular type.
