The galaxy presents as a likely interacting system. It is composed of two distinct, gravitationally interacting galactic bodies. The primary component displays a relatively smooth, elliptical morphology with a yellowish-orange hue, suggesting an older stellar population. The secondary component, located in close proximity to the primary galaxy, exhibits a bluer color, indicating a younger, hotter stellar population, which may be indicative of recent star formation activity, perhaps triggered by the gravitational interaction between the galaxies. There appears to be some tidal distortion present, though not severely pronounced. The overall system appears to be in a relatively early stage of merging.
