The galaxy appears as an elliptical or spheroidal structure, exhibiting a smooth light distribution. The central region displays a concentrated luminosity profile, potentially indicating a dense stellar population or the presence of an active galactic nucleus, although the resolution is insufficient to confirm. The overall color suggests an older stellar population, likely dominated by evolved red giant stars. There is no discernible disk component or spiral arm structure. The morphology is generally regular, without significant tidal features or distortions, suggesting minimal recent interaction with other galaxies.
