The galaxy presents a relatively smooth, elliptical morphology with an apparent lack of distinct spiral arms. It appears to be undergoing a significant merger event, exhibiting tidal disturbances and distorted features. There is a prominent central bulge with a high degree of circularity. The galaxy displays a mixture of light that is consistent with intermediate-age to older stellar populations. Some regions show evidence of recent or ongoing star formation, but at a low rate. Overall, the galaxy has undergone at least one major interaction and is likely in the late stages of a major merger.
