The galaxy appears to be a relatively smooth, centrally concentrated object with a roughly elliptical morphology. The light profile suggests a bulge-dominated system.  There is a bright, yellowish core that fades outward to a diffuse halo of blueish light, hinting at a population of younger stars in the outer regions. Overall, the galaxy exhibits a lack of prominent spiral arm structure or strong dust lanes. There are hints of a subtle disturbance in the outer halo. The overall appearance suggests a mature galaxy, possibly in the process of transitioning from a spiral to an elliptical morphology.
