The galaxy presents a generally smooth, elliptical morphology. It is characterized by a central bulge that appears largely spheroidal and is concentrated in the middle of the galaxy. There is faint extension of what appears to be a disk around the central bulge. The color profile suggests a stellar population that is generally older, with a slight population of younger stars on the outer edges of the disk, which might be indicative of ongoing, but low-level, star formation in the outer regions. There is no clear indication of tidal disturbances or major mergers, though minor asymmetries could imply past interactions or minor disturbances.
