The galaxy presents as a centrally concentrated object, exhibiting a smooth, elliptical morphology. A bright, relatively compact nucleus is visible, which fades gradually outward into the galaxy's halo. The overall color profile suggests a population of older stars dominating the light output, but the greenish hue may indicate some ongoing, though modest, star formation within the disk or halo. The galaxy's shape appears to be somewhat flattened, rather than perfectly spherical, suggesting a possible disk component viewed at an oblique angle. There is no obvious evidence of significant disturbances or merging activity.
