The galaxy presents as a somewhat elliptical, though nearly round, structure. It has a bright, concentrated central bulge with a yellow-orange hue, indicating an older stellar population. There is a fainter, bluer disk component surrounding the bulge, suggesting some ongoing star formation within the galaxy. Faint features may indicate either a recent minor disturbance or very early signs of a merger event, though generally the galaxy appears relatively undisturbed. The overall smooth appearance suggests a well-evolved system, consistent with a galaxy undergoing moderate star formation.
