The galaxy appears to be elliptical in shape, exhibiting a smooth, largely featureless morphology. The central region displays a concentrated luminosity gradient, suggesting a dense stellar population or active galactic nucleus. The color profile shifts from a bright, slightly redder core to a more subdued, bluer halo region, potentially indicating a difference in stellar populations with the core having an older, redder population and the outer regions a younger, bluer one. There is no clear evidence of spiral arms or a prominent disk structure. The lack of significant morphological disturbances suggests it is not currently undergoing a major merger event. Overall, the galaxy presents as a relatively quiescent, evolved system.
