The galaxy presents a predominantly smooth morphology, appearing largely featureless upon visual inspection. Its shape approximates a circular form. There is no obvious spiral arm structure or bar. The color profile suggests a central concentration of older stars, indicated by the reddish hue. The outer regions exhibit a slightly bluer tint, potentially suggesting the presence of a younger stellar population, but this is not definitive given the image resolution. There's no immediately apparent evidence of ongoing merger activity or tidal disturbances; the galaxy appears relatively undisturbed. Overall, the galaxy is likely an elliptical, with a smooth, well-defined structure.
