The galaxy appears as a centrally concentrated object, with a somewhat smooth, diffuse morphology. It exhibits an elliptical shape, slightly elongated along one axis. The color gradient suggests a population of older stars dominating its light output, giving it a yellowish-red hue in the center. This color is somewhat consistent throughout the galaxy, except for a slightly yellower, brighter center. There also appears to be some evidence of possible merger activity in the form of a tidal tail or minor disturbance. The outer regions of the galaxy fade gradually into the background, with no distinct or sharp edges.
