The galaxy appears as a centrally concentrated object with a smooth, round morphology. It exhibits a dominant orange hue, indicative of an older stellar population. There is some indication of a possible companion galaxy that is smaller and less massive than the other, and has a similar orange hue. No spiral arm structures or significant dust lanes are visually apparent. Based on color, morphology, and lack of visible star forming regions, this galaxy seems to be a well evolved galaxy that could be classified as an elliptical. The galaxy does not appear to be experiencing any major mergers or significant disturbances in its structure.
