The galaxy presents a generally elliptical morphology with a smooth, diffuse appearance. The central region is characterized by a concentration of light, suggesting a possible nucleus or bulge. The light is redder in the center. There are subtle hints of arm-like structures extending from the core, though they are not sharply defined. These features imply the galaxy is likely a spiral galaxy. The lack of strong dust lanes or prominent star-forming regions suggests a relatively low rate of current star formation. There are suggestions of merging, though no major disturbance. The color distribution implies a relatively old stellar population.
