The galaxy presents a relatively smooth, somewhat elliptical morphology. There is a slight elongation, but it appears mostly round.  The central region exhibits a bright, concentrated luminosity. No distinct spiral arm structures or prominent dust lanes are readily apparent in the visible bands. There may be a slight hint of tidal disturbances or a minor merger event. The galaxy has intermediate color values between the green, red and infrared bands. This suggests there is ongoing star formation but it is not particularly intense, and is dominated by older stellar populations.
