The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. A dominant, bright core emanates light across all observed wavelengths, suggesting an older stellar population. The overall color appears slightly reddish, indicative of minimal current star formation. There is a subtle asymmetry in the outer regions of the galaxy, potentially caused by a past or ongoing minor interaction. This asymmetry is seen as a slightly more extended halo on one side of the galaxy. No prominent dust lanes or spiral arm structures are discernible. The galaxy's shape is generally round, exhibiting a smooth luminosity profile that declines gradually from the center. Faint, diffuse light extends outwards, indicating a relatively large galactic halo.
