The galaxy appears as a concentrated, elliptical-like object. The central region exhibits a bright, yellowish hue, suggesting an older stellar population and potentially a significant bulge component. Moving outward from the core, the light intensity diminishes gradually, with the color transitioning towards a slightly redder shade. The overall structure seems relatively smooth, lacking any prominent spiral arms or significant dust lanes visible in this image. There may be a slight irregularity in the surrounding halo of the galaxy, suggesting that it may be in the beginning stages of a merger with another galaxy.
