The galaxy presents a generally smooth, elliptical morphology with a high degree of central concentration. The light distribution appears relatively uniform, lacking any distinct spiral arm structures or prominent dust lanes. The color gradient suggests a population of primarily older stars, with the central region exhibiting a slightly yellowish hue, indicative of a dominant population of evolved stars. The outer regions show a subtle shift towards bluer tones, potentially indicating some ongoing, but limited, star formation activity. The overall structure indicates the system is likely nearing the end of its major star-forming phase. No signs of recent or ongoing mergers or tidal disturbances are discernible, suggesting the galaxy has been relatively isolated and undisturbed for a significant period. The observed features are consistent with a passively evolving elliptical galaxy.
