The galaxy appears as a diffuse, elliptical-shaped object. The light distribution is concentrated towards the center, exhibiting a smooth gradient outwards with no distinct spiral arm structures visible. The color profile suggests a relatively older stellar population, with a dominant yellowish-red hue. There are hints of bluer components, particularly at the galaxy's periphery. The galaxy presents a fairly regular morphology with a small irregularity, possibly indicative of minor interactions or internal disturbances. No prominent dust lanes or active galactic nucleus features are discernible within the resolution limits. It seems as though the galaxy has a relatively low star formation rate.
