The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge, transitioning into a more diffuse halo. There is a slight elongation, indicating a deviation from a perfectly circular shape. The color profile suggests an older stellar population. A redder hue dominates the central region, likely indicative of evolved stars. Some bluer regions are seen within the galaxy. The galaxy exhibits a relatively low rate of star formation and would appear to be a rather massive galaxy, based on its brightness. Possible minor interaction with a smaller galaxy. 
