The galaxy presents as a roughly elliptical, relatively smooth structure with a concentrated central bulge exhibiting a yellowish hue. The outer regions appear slightly bluer, suggesting a younger stellar population compared to the core. There is no apparent spiral arm structure or significant dust lane obscuration visible in this image, lending to a classification leaning towards an early-type galaxy, potentially an elliptical or lenticular galaxy. There is a slight elongation in the shape, but it is mostly round, and the lack of any clear disturbances suggests it is not currently undergoing any major merging events. Overall, the galaxy seems to be a mature system with ongoing, but relatively low, star formation in its outer regions.
