The galaxy appears as a roughly elliptical, concentrated source of light. Its core exhibits a bright, yellowish-white hue, indicating a high density of stars, possibly older stellar populations. Moving outwards from the core, the light gradually diminishes, and transitions to a more diffuse, yellowish color, characteristic of a stellar halo. There is no evident spiral arm structure or distinct dust lanes visible. The overall smooth appearance suggests that this is either an elliptical galaxy or a lenticular galaxy viewed face-on. No signs of recent or ongoing major merger events or tidal disturbances are visible. The galaxy seems to be relatively isolated and undisturbed.
