The galaxy appears as a relatively smooth, centrally concentrated object. It exhibits a subtle disk-like morphology, though the features are not particularly prominent, with no obvious spiral arm structure visible. The galaxy's color gradient suggests a population of primarily older stars throughout, though there are subtle differences in stellar population. The central region appears slightly brighter and bluer, potentially indicating a younger stellar population or ongoing star formation in the galactic nucleus. There is a lack of significant dust lanes or prominent star-forming regions within the galaxy, suggesting it is not undergoing intense starburst activity. There may be faint tidal features surrounding the galaxy, indicating a past interaction or merger event. The overall appearance indicates a massive galaxy with a mature stellar population, potentially on the transition towards a lenticular or elliptical type.
