The galaxy appears to be an elliptical or lenticular type, characterized by a centrally concentrated bulge. It displays a smooth, relatively featureless morphology. The core of the galaxy exhibits a high degree of luminosity, suggesting a dense stellar population or potentially an active galactic nucleus. A small, slightly off-center region shows hints of yellower light, which may indicate an older population of stars, or perhaps dust absorption. The main body of the galaxy exhibits a somewhat round structure. There are subtle irregularities that suggest a possible past interaction, but overall the system appears fairly relaxed.
