The galaxy presents as a relatively smooth, elliptical structure. The core region exhibits a concentrated luminosity, appearing bright and yellow in color, suggestive of an older stellar population. Moving outward from the core, the luminosity decreases gradually, with a more diffuse, reddish-tinged halo extending further. There is a slight disk-like shape present, but the galaxy overall is mostly spheroid. No prominent spiral arms or dust lanes are discernible. There are subtle signs of recent interactions and perhaps an ongoing merger. The lack of distinct features like spiral arms and the predominantly redder color imply a relatively low current star formation rate.
