The galaxy presents as a relatively compact, elliptical object. Its light is predominantly blue, suggesting the presence of a population of younger, hotter stars. The object displays a smooth, centralized light distribution, with brightness diminishing gradually from the center, indicative of an older stellar population dominating the galaxy. It has a moderate degree of roundness, not appearing particularly flattened or elongated. No spiral arms or distinct disk features are discernible. There is slight evidence of disturbance in the galaxy's morphology, however it appears the galaxy is isolated without any major mergers occurring. Overall star formation is very low within the galaxy.
