The galaxy presents an elliptical morphology, with a smooth, centrally concentrated light distribution. The core region exhibits a bright, yellowish hue, indicative of an older stellar population. Fainter, diffuse extensions of light are observed surrounding the core, suggesting a gradual decrease in stellar density with increasing radial distance. There is a subtle indication of a disk structure in the galaxy. Additionally, there are slight disturbances and subtle color variations within these outer regions. The overall color profile suggests a relatively low rate of current star formation.
