The galaxy presents a mostly smooth, elliptical morphology, with a high concentration of light in the central region. There is a small, separate object that is likely interacting with the main body of the galaxy and causing some form of disturbance. The galaxy exhibits a yellow/red hue. This is likely the signature of an older stellar population. The primary body of the galaxy appears elongated, indicating a relatively high ellipticity, with a major axis extending generally in a northeast-southwest direction. The object is compact, with no clear evidence of spiral arms or prominent dust lanes visible.