The galaxy presents as a relatively smooth, elliptical-like structure. It lacks distinct spiral arms or a prominent disk. The light distribution is centrally concentrated, exhibiting a bright core that fades gradually outwards into a more diffuse halo. There's a subtle elongation visible, indicating a slight deviation from perfect circularity. No major disturbances or signs of an ongoing merger are immediately apparent, although there might be subtle irregularities in the outer regions that could suggest minor tidal interactions. The overall color appears relatively uniform, tending towards the redder end of the spectrum, which is consistent with a population of older stars and reduced star formation activity.
