The galaxy presents a generally smooth and rounded morphology. The central region exhibits a concentrated, bright, yellowish core, suggesting a relatively older stellar population and possibly a supermassive black hole. This brighter core gradually fades into an extended, diffuse halo, encompassing a significant portion of the galaxy's structure. There is a subtle color gradient from the inner regions outwards, with the outer areas displaying a slightly bluer hue, potentially indicative of ongoing, albeit subdued, star formation activity. Overall, the structure appears largely undisturbed, lacking any significant signs of tidal interactions or major mergers. Minor disturbances might be present, but the overwhelming impression is that of a settled, relatively quiescent system.
