The galaxy presents a largely smooth morphology, appearing elliptical or lenticular in shape. It exhibits a centrally concentrated light distribution, with the core appearing bright and diffuse. There is a distinct lack of discernible spiral arms or prominent dust lanes. The overall color appears relatively red, suggesting an older stellar population, lower star formation rate, and/or significant dust content. There is also a very small amount of evidence of disturbances, but it is likely not currently undergoing a major merger event. The system is generally round with minimal elongation.