This galaxy presents a centrally concentrated morphology. It appears to be a relatively smooth, somewhat elliptical structure. The core exhibits a bright, yellowish-white hue, suggesting a concentration of older stellar populations and possibly a supermassive black hole. The light gradually diffuses outwards from the core into a more diffuse halo. There is a subtle shift in color in the outer regions toward bluer tones, implying a presence of younger, hotter stars though not as clearly demarcated as spiral arms, instead suggesting general star forming regions. There are also light distortions near the galaxy. I see a slight asymmetry. There does not appear to be evidence of a major ongoing merger or significant tidal disruption, though the slight asymmetries might hint at a minor past interaction.
