The galaxy presents as a relatively smooth object with a somewhat elliptical morphology. The core region exhibits a high degree of luminosity, with a gradual decrease in brightness observed towards the outer edges. It appears to be in a relatively isolated environment, showing no obvious signs of recent or ongoing major merger activity, although a minor disturbance cannot be ruled out. The galaxy's overall color is indicative of an older stellar population, suggesting a possible lack of significant recent star formation within the main body of the galaxy.
