The galaxy presents a largely smooth, elliptical morphology, exhibiting a high degree of central concentration. The light distribution suggests a well-defined nucleus, surrounded by a diffuse, extended halo. The overall color appears relatively red, consistent with an older stellar population and a relatively low rate of on-going star formation. There is no strong evidence of spiral arms or significant dust lanes. The galaxy appears relatively undisturbed, showing no clear signs of a recent major merger or tidal interactions. The isophotes appear close to circular. There is a slight suggestion of bluer light in the outer regions, but further investigation would be required to assess its significance.
