The galaxy presents a generally smooth and rounded morphology. There is evidence of a slight disc-like structure, but it is not highly pronounced. No significant spiral arm structure is observed. The color profile suggests a dominant older stellar population with a redder hue. There is a possible tidal disturbance, although this could just be the resolution of the image. The estimated half-light radius suggests that the galaxy is relatively compact. The general appearance indicates an elliptical galaxy or a lenticular galaxy that is not highly inclined to our line of sight. Star formation appears to be relatively low.
