The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology, appearing somewhat rounded with a slight elongation. The color profile suggests a predominantly older stellar population, evidenced by the reddish-yellow hue of the central bulge, indicating a lack of significant recent star formation in that region. The outer regions of the galaxy are bluer, potentially signifying the presence of younger stars or ongoing, albeit low-level, star formation. No prominent spiral arms or distinct features such as dust lanes are discernible. There are no visible signs of tidal disturbances or interactions with other galaxies. The galaxy shows a degree of symmetry, with a gradual decrease in light intensity from the center outwards.
