The galaxy presents as a generally smooth, elliptical-like structure. The galaxy's core exhibits a concentration of light, appearing relatively bright and slightly yellowish-orange in hue. The light gently diffuses outward from the core, lacking any prominent spiral arm structures or distinct features typically associated with disk galaxies.

There is some slight mottled color variation in the outer regions, indicating some localized star formation. This activity seems to be concentrated in a few faint patches rather than being uniformly distributed. The overall color suggests an older stellar population, with some hints of ongoing star formation that is possibly weak.

The rounded shape is apparent, with no significant tidal disturbances or distortions suggestive of recent major merger events. There is a very slight asymmetry observable, with the light being more concentrated on one side of the core than the other.
