The galaxy presents as a relatively smooth, elliptical-like structure. Its core exhibits a bright, concentrated luminosity, potentially indicating a high density of stars or an active galactic nucleus. Moving outward from the core, the intensity of light diminishes gradually. Faint, diffuse extensions surround the central region, suggesting a halo of older stars. No distinct spiral arms or bar features are apparent. The galaxy appears somewhat compact, implying a relatively low star formation rate and a greater age compared to spiral galaxies with prominent star-forming regions. There is no obvious sign of any tidal disturbances or ongoing mergers.
