The galaxy presents as a luminous, elliptical form. The central region exhibits a bright, concentrated core, suggesting a high density of stars in this area. The overall color profile indicates a relatively older stellar population, with a tendency toward redder wavelengths. The galaxy appears largely smooth in texture, with no obvious spiral arm structures or significant dust lanes visible. The shape is somewhat elongated, deviating from a perfectly circular form. There is some indication of minor disturbances or interactions, possibly evidenced by subtle asymmetries or distortions in the outer regions. Overall, it seems to be a well-evolved galaxy undergoing minimal active star formation at the time the light was emitted.
