The galaxy exhibits a generally smooth, elliptical morphology. Its light is centrally concentrated, with the intensity gradually decreasing outwards from the nucleus. The galaxy appears to be relatively compact, lacking any prominent spiral arms or significant disk structure. The color profile suggests an older stellar population with a dominant redder hue, with the center appearing nearly white, and the outer regions showing hints of blue. This would indicate that younger stars reside in the outskirts of the object. There are no indications of major mergers or tidal disturbances.
