This galaxy presents as a relatively smooth object, with a bright central bulge indicative of an older stellar population. There appears to be a weak disk component, evidenced by a slight elongation. There's a hint of spiral structure, but it is subtle and may be due to arms that are tightly wound. The color profile suggests a moderate amount of star formation is occurring, but it may be at lower levels. No obvious major merger events or significant tidal disturbances are observed. The galaxy is more elliptical, and is most likely a lenticular galaxy type.
