The galaxy presents a flattened, elliptical morphology. The central region exhibits a concentrated, yellowish-orange hue, suggesting an older stellar population likely dominated by evolved stars. This core is surrounded by a more diffuse, greenish halo. This halo indicates the presence of a younger stellar population and possibly ongoing star formation. The overall shape is predominantly smooth, with no immediately obvious signs of major disturbances or merging activity, though minor irregularities cannot be ruled out at this resolution. There are no distinct spiral arms visible.
