The galaxy presents as an elliptical morphology, exhibiting a smooth, relatively featureless light distribution. The central region is characterized by a concentrated, bright core which gradually decreases in surface brightness outwards. The color profile shifts from a more yellow-white hue in the nucleus to a redder shade in the outer regions of the galaxy. This suggests an older stellar population dominating the outer regions. The overall shape is elongated but not highly so, approximating an in-between stage between round and cigar-shaped. There is no apparent indication of spiral arms or significant dust lanes. Similarly, there are no strong visual signs of an ongoing or recent major merger event, though a minor disturbance is not easily ruled out.
