The galaxy presents as a relatively smooth, centrally concentrated object, approximately elliptical in shape with a hint of slight elongation. The core exhibits a bright, yellowish hue, possibly indicative of an older stellar population. Moving outwards from the core, the color transitions to a more diffuse, bluish-white halo. This could suggest a younger stellar population within the outer regions, indicative of some ongoing, albeit potentially low-level, star formation. There is no evidence of distinct spiral arms or a prominent disk structure. No significant morphological disturbances are apparent, suggesting the galaxy is relatively isolated and has not recently experienced a major merger event. Overall, this galaxy appears to be a relatively quiescent, moderately massive system in the distant universe.
