This galaxy presents an elliptical morphology with a bright, concentrated nucleus. The core exhibits a pronounced blue hue, possibly indicating a population of young, hot stars or a contribution from an active galactic nucleus. Surrounding the core, a more diffuse, greenish halo is visible, suggesting a broader distribution of older stellar populations. There are subtle indications of faint tidal features or minor disturbances extending from the main body of the galaxy, particularly at the periphery. The structure is compact with a relatively smooth appearance, though faint irregularities suggest a possible interaction or recent merger. The galaxy lacks clearly defined spiral arms or a prominent disk structure. Overall, it appears to be an early-type galaxy, with a potential recent interaction event.
