The galaxy presents as an elliptical morphology, exhibiting a smooth, featureless appearance. Its overall shape is elongated with a noticeable bulge dominating the central region, which appears significantly brighter than the outer regions of the galaxy. The color profile is generally redder, indicative of an older stellar population with relatively little ongoing star formation. There is no strong evidence of spiral arms or a distinct disk structure visible in the imagery. The light appears to smoothly fade from the central bulge towards the edges of the galaxy.
