The galaxy presents as a relatively compact object. It displays a generally elliptical morphology with a high degree of central concentration. The light profile appears smooth, suggesting an evolved stellar population. The core exhibits a yellowish hue, potentially indicative of older, cooler stars. There is some evidence of bluer light concentrated in a region that could be an area with ongoing star formation. Overall, the galaxy does not exhibit any obvious signs of major disturbances or interactions. The shape is predominantly round, with minor deviations from perfect circularity.
