The galaxy presents as a diffuse, elliptical-shaped structure with a relatively smooth light distribution. There is a notable concentration of light toward the center, suggesting a prominent galactic nucleus or bulge. The overall color appears slightly blueish, hinting at a population of younger, hotter stars, though this is subtle. The galaxy's shape is elongated with no clear spiral arm structures visible. There's no obvious sign of significant ongoing merger activity, though there may be some minor asymmetries in the outer regions that could suggest minor tidal interactions or internal disturbances.
