The galaxy presents a generally elliptical morphology, appearing largely smooth and spheroidal. The core exhibits a high surface brightness with a yellowish hue, suggestive of an older stellar population. Moving outward from the core, the light gradually diffuses, forming an extended halo with some subtle color variation. Faint bluish tints are observed in the outer regions of the halo, which could indicate the presence of younger, hotter stars. No distinct spiral arms or a prominent disk structure are apparent. There is no obvious indication of any recent major merger activity, although there appears to be a slight irregularity in the outer regions. Based on these observations, the galaxy is likely a massive elliptical galaxy at a moderate redshift.
