The galaxy presents an elliptical morphology, appearing as a smooth, concentrated distribution of light. The core region exhibits a high degree of luminosity, with a discernible gradient decreasing outwards towards the halo. The halo is extended, but also appears relatively featureless. There are no strong signs of spiral arm structures. The shape is closer to "in between" round and cigar shaped with some elongation. There is no obvious indication of a major merger event or significant tidal disturbances, though minor disturbances cannot be ruled out. The galaxy's color is a yellow-orange hue, suggestive of an older stellar population and relatively low ongoing star formation.
