The galaxy presents a generally smooth, elliptical morphology, although subtle internal features suggest it is not perfectly featureless. It has an overall yellowish-orange hue, indicative of an older stellar population and/or significant dust obscuration. The light is concentrated toward the center, decreasing gradually towards the outer edges. There appears to be a slight elongation, it is mostly rounded but slightly oval. A minor disturbance or interaction may be inferred from the general structure and color distribution. There is no clear evidence of a distinct disk component. The overall appearance suggests an evolved galaxy with a substantial mass. Star formation appears to be low within the galaxy. There is a possibility of a minor merger event in the galaxy's recent history.
