The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central region, gradually fading in intensity towards its outer edges. There are no distinct spiral arms or pronounced dust lanes visible. The galaxy appears slightly elongated, but predominantly round. The color profile suggests a population of older stars, with a general reddish-orange hue. There is a slight hint of bluer light in the outermost regions of the galaxy. There is no evidence of an ongoing major merger.
