The galaxy presents a disturbed morphology, likely undergoing a merger event. A primary, relatively smooth central component is visible, appearing somewhat elliptical. A secondary, smaller component is observed nearby, exhibiting a less defined structure. There is evidence of tidal distortions or possible tidal tails extending from the galaxy indicating interactions between multiple galactic components. Overall, the galaxy presents a relatively compact appearance with a yellowish-orange hue. This color suggests a population of older stars and moderate levels of star formation. The galaxy's shape is noticeably non-spherical, indicating an ongoing disruption of its structure.
