The galaxy presents as a system undergoing a significant interaction or merger. One primary component appears to be a relatively smooth, spheroidal galaxy with a diffuse halo. The second prominent component seems to be a distorted spiral arm, or a tidal tail, originating from what appears to be a highly disturbed disk galaxy. This arm exhibits a reddish hue suggesting a population of older stars and/or significant dust obscuration. The overall color index of the system suggests the presence of both young, blue stars and older, redder stellar populations. Morphological analysis suggests that the system may be experiencing a minor disturbance or an ongoing merger event.
