The galaxy presents a largely smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile, with intensity decreasing radially outwards. There are no apparent spiral arm structures or significant dust lanes visible in the image. The galaxy appears to be a relatively regular spheroid, with no signs of major mergers or tidal disturbances. It exhibits a yellowish hue, suggesting a relatively older stellar population with a diminished rate of ongoing star formation. There is little indication of intense, recent star formation, as evidenced by the lack of blue or ultraviolet light. Overall, the morphology suggests a galaxy dominated by older stars with minimal active star formation, typical of an elliptical or S0 galaxy at its estimated redshift.
