This galaxy appears to be a relatively smooth elliptical galaxy, exhibiting a high degree of central concentration. It has a pronounced bulge that dominates its overall luminosity. The light distribution appears to be quite uniform throughout the galaxy. There is a potential indication of a minor disturbance in the galaxy’s morphology which is most likely not a major merging event. The galaxy is slightly elongated, but mostly spherical in shape. 

The color index suggests the presence of an older stellar population, but there may be some evidence of ongoing, albeit low, levels of star formation within the galaxy. 
