The galaxy presents an elliptical morphology, exhibiting a generally smooth light distribution without obvious spiral arm structures. The core is concentrated, with a yellow-white color, suggesting an older stellar population and a relatively low rate of star formation in the central region. The galaxy shows a gradual decrease in surface brightness from the core outwards, with a more diffuse and slightly bluer outer halo or envelope. There is subtle irregularity in the outer regions, hinting at potential minor tidal interactions or past mergers. Overall, the galaxy appears to be an evolved system.
