The galaxy presents an elliptical morphology, with a high degree of central concentration. The core region exhibits a bright, yellowish-white luminosity, indicative of a high density of older stellar populations. The galaxy appears relatively smooth in structure, lacking prominent spiral arms or significant dust lanes. A subtle decrease in the stellar density is observed as we move outwards towards the galaxy's halo. The light profile suggests that the galaxy has undergone a significant amount of merging. The slight asymmetry indicates a potential recent minor merger event or tidal interaction. The galaxy appears relatively isolated, suggesting that environmental effects might not be a primary driver of its evolution. A very faint outer halo is visible.
