The galaxy presents as a relatively smooth, elliptical-like structure. The core of the galaxy displays a concentrated luminosity, appearing bright yellow, suggesting a population of older stars dominating the central region. The luminosity gradually diminishes outwards, forming a halo of diffused light. There is no obvious structure, such as spiral arms or a prominent disk. Faint hints of redness are present around the central core, possibly indicating the presence of dust or older stellar populations. The overall shape appears somewhat rounded, lacking any significant elongation. It shows no evidence of ongoing merging events or tidal disturbances.
