The galaxy presents as a relatively compact, elliptical-like structure. It exhibits a centrally concentrated brightness profile, fading smoothly towards its outer regions. The core region appears to be a bright, relatively uniform in color, suggesting a concentration of older stellar populations. The galaxy appears mostly smooth in texture with minimal signs of active star formation. Its shape is close to circular. No significant signs of tidal distortions or interactions with other galaxies are immediately obvious, indicating a state of relative isolation and gravitational stability. Overall, this galaxy is a relatively old and inactive galaxy.
