The galaxy presents as a relatively smooth and concentrated object. The central bulge appears prominent and exhibits a yellowish hue, suggesting a population of older stars.  There is little evidence of spiral arm structure. The overall shape is elliptical or possibly a lenticular disk with an inclination near face-on.  The galaxy appears undisturbed, showing no signs of tidal tails or distortions indicative of a recent major merger event, although a minor disturbance cannot be ruled out. Faint extensions of light are visible extending from the central region, however this is quite minimal. The galaxy is estimated to be a significant mass and moderate amount of recent star formation. 
