The galaxy exhibits a generally smooth morphology. It appears elliptical in shape, with a concentrated central bulge. The color profile suggests an older stellar population, as evidenced by the redder hues concentrated in the core, transitioning to slightly bluer tones in the outer regions. There are no apparent spiral arms or significant dust lanes visible. The galaxy shows no obvious signs of recent or ongoing major merger activity or strong tidal disturbances. A slight elongation is observed, however the galaxy has no noticeable features.
