The galaxy presents as a relatively smooth, elliptical-like object. Its morphology appears dominated by a spheroid component with a high degree of central concentration. The light profile exhibits a gradual decline in surface brightness from the core outward, with no prominent spiral arms or bar structures visible. The overall color is indicative of an older stellar population, suggesting a lower ongoing rate of star formation. The galaxy displays a round shape with very minimal disturbances. There is no indication of any major merging events. The galaxy has a relatively high mass with intermediate star formation. 
