The galaxy appears as a centrally concentrated, luminous object. It exhibits a relatively smooth, elliptical morphology with little to no discernible substructure. The color profile suggests a dominance of older stellar populations, with a higher concentration of redder light. The overall round shape indicates minimal tidal distortion, suggesting the absence of major ongoing mergers or significant gravitational interactions. Faint extensions around the central region may be a sign of a stellar halo or tidal streams from minor disturbances.
