The galaxy appears as a centrally concentrated, relatively smooth and rounded object. Its light profile suggests a dominant bulge component, with an apparent lack of well-defined spiral arm structures or significant dust lanes. The central region displays a slightly brighter, more condensed core, potentially indicative of an active galactic nucleus or a high concentration of stars. The galaxy's color suggests a moderately evolved stellar population, with a mix of blue and redder hues, without a strong presence of very young, intensely star-forming regions. Based on the faint distortions in the outer regions of the galaxy, it has likely undergone a minor merging event. Overall, the galaxy appears to be an elliptical galaxy.
