The galaxy presents as a single, largely featureless object. It exhibits a centrally concentrated luminosity profile, suggesting a significant bulge component. The overall shape approximates a rounded morphology, with a slight deviation towards an elliptical form. The color gradient transitions from a bright, relatively blue-white core region to a more diffuse, slightly redder outer halo. This color variation might be indicative of differential stellar populations, with younger, bluer stars dominating the core and older, redder stars populating the outer regions. There is no clear evidence of spiral arm structure or other distinct morphological features within the visible portion of the galaxy. There is some indication of a minor disturbance in the galaxy, but it is difficult to determine the source of this disturbance. Overall, the object appears to be consistent with an elliptical or lenticular galaxy at its redshift.
