The galaxy presents as a centrally concentrated object with a generally smooth morphology. The core exhibits a bright, reddish hue, indicating a likely population of older stars. Fainter, greenish-yellow light emanates from the surrounding regions, potentially indicative of ongoing, albeit subdued, star formation or a mix of stellar populations. There is a slight elongation to the galaxy's shape. The smoothness of its appearance suggests a lack of major disruptive events or active merging processes. Overall, the galaxy appears to be a relatively undisturbed system, potentially an elliptical galaxy.
