The galaxy appears to be an elliptical galaxy with a smooth, concentrated light profile. Its color is primarily yellowish-white, suggesting an older stellar population with a relatively low rate of on-going star formation. There is no apparent disk structure or spiral arm morphology, and the galaxy exhibits a high degree of circular symmetry. No signs of active galactic nuclei or significant dust lanes are observed. The object appears relatively isolated and there is no apparent evidence of merging activity. The galaxy's overall visual impression is that of a quiescent, passively evolving system.
