The galaxy appears as an elliptical morphology, exhibiting a generally smooth light distribution. The galaxy presents an elongated shape, with a discernible major axis significantly longer than its minor axis. A central bulge is prominent and appears brighter and more concentrated than the outer regions. There is a subtle color gradient, with the central bulge appearing more yellow/orange, potentially indicative of an older stellar population. The outer regions have a bluer tint. There is no apparent spiral structure or dust lanes visible within the galaxy. There's no obvious interaction or recent merger activity. The galaxy seems isolated and undisturbed.
