The galaxy presents as a relatively smooth, centrally concentrated object with a slightly elliptical morphology. The core region exhibits a bright, yellowish-white hue, suggestive of an older stellar population dominating the central bulge. Moving outward from the core, the galaxy appears to transition to a more diffuse and slightly bluer appearance, with an inclination angle slightly off from being a perfect circle. This color shift may indicate the presence of younger stars within the galaxy's disk or outer regions. There are no obviously discernible spiral arm structures. There is no evidence of any active galactic nuclei or star formation in this galaxy. Overall, the galaxy has a smooth appearance indicative of an elliptical galaxy.
