The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. There is a marked concentration of light towards the galactic center, exhibiting a bulge-like structure. The color appears generally redder, suggesting an older stellar population and potentially lower star formation activity. There is only the faintest evidence of a disk component; instead, the light distribution is characterized by a high degree of rotational symmetry. Weak tidal features are also visible, indicating minor gravitational interactions. Overall, the galaxy is a mature system with minimal recent or ongoing star formation.
