The galaxy presents a largely smooth, elliptical morphology. There is a slight elongation, but it is primarily round in appearance. Its color profile suggests a dominant population of older stars, contributing to the overall reddish-yellow hue. While a faint disk structure cannot be entirely ruled out, there is no prominent spiral arm structure visible, leading to its characterization as smooth. There are no signs of major disturbances or ongoing mergers, although minor disturbances in the galaxy's structure cannot be entirely dismissed. The galaxy possesses a substantial mass.
