The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a concentrated, bright core that gradually diffuses outwards. The light distribution is fairly uniform without prominent spiral arm structures or distinct dust lanes. There is a subtle color gradient observed, transitioning from a yellow-white hue at the center to a slightly redder color in the outer regions. This could indicate an older stellar population dominating in the outer parts of the galaxy. There appear to be no major disturbances to the galaxy's structure, like tidal tails or distortions that would suggest it is currently merging with another galaxy. Overall, it appears to be a well-formed, relatively undisturbed galaxy.
