The galaxy appears to be an elliptical galaxy with a smooth, featureless morphology. Its overall shape is elongated, being roughly half as wide as it is long. The galaxy has a prominent central bulge that is bright and concentrated with what appears to be older stars. There is a decrease in luminosity as it gets farther from the center, although a faint halo surrounds the bulge. There are subtle color gradients, with the central regions exhibiting a yellowish-orange hue, suggesting an older stellar population, transitioning to slightly bluer tones in the outer regions, implying the presence of some younger stars or a low level of ongoing star formation. The galaxy shows no evidence of spiral arms or disk structure within this image. There is no clear indication of ongoing merger activity, and it is difficult to discern much about the structure of the outer edges of the galaxy from this image.
