The galaxy exhibits a morphology suggestive of an ongoing or recent interaction/merger event. Two primary components are visible: a larger, more luminous central body, and a smaller, less luminous secondary component. The larger component displays a relatively smooth light distribution. The smaller component appears more elongated. There is a hint of tidal features or faint, extended structure surrounding the galaxy, possibly indicating gravitational disturbance. The color indices imply a mixture of stellar populations, likely with a significant population of older stars. The galaxy's overall shape is somewhat elliptical.
