The galaxy presents a generally elliptical morphology with a relatively smooth light distribution, indicative of a system dominated by an older stellar population. The major to minor axis ratio suggests the galaxy is somewhat flattened, but not highly elongated. The galaxy's color profile transitions from slightly bluer hues in the central region to redder tones in the outer regions, potentially indicating a radial gradient in stellar population age or dust content. There is a slight asymmetry in the outer isophotes, potentially suggestive of a minor interaction or merger history, although no major disturbances are readily apparent in the image. Overall, the galaxy appears to be a relatively undisturbed early-type system at a moderate redshift.
