The galaxy presents as a relatively smooth, elliptical-like structure. Its core is a bright, concentrated region with a yellowish hue, indicating an older stellar population. The light gradually fades from the center outwards, suggesting a decreasing stellar density. There is little to no observable structure such as spiral arms or a defined disk. The galaxy appears to be a settled system with no signs of ongoing major mergers. Faint bluer regions are possibly present towards the outer edges, this could potentially indicate areas of more recent star formation. Overall, the galaxy's morphology indicates a evolved system.
