The galaxy presents as a somewhat elliptical or lenticular structure. Its central region exhibits a bright, concentrated core that appears yellowish, possibly indicating an older stellar population. The light becomes fainter toward the outer regions of the galaxy. There is little evidence of distinct spiral arms or a well-defined disk structure within the galaxy. The overall appearance is smooth and lacks pronounced features or irregularities. A subtle hint of redder hues exists on the periphery. The galaxy has a moderate level of ellipticity, appearing neither perfectly spherical nor extremely elongated. There is no obvious sign of any recent major merger events. The galaxy appears relatively undisturbed.
