This galaxy appears as a relatively compact and luminous object. It exhibits a generally smooth morphology with a dominant, rounded central bulge. There is little evidence of spiral arm structures or distinct features, giving it a lenticular or elliptical-like appearance. The galaxy displays a color gradient, with a reddish hue concentrated in the central regions, transitioning to bluer colors in the outer parts. This may indicate a population of older stars in the core, with younger, bluer stars present in the disk or halo. There might be a ring-like structure present or the start of a spiral formation. Based on this, there is most likely ongoing star formation and a considerable mass associated with this system. No obvious signs of recent major merger events are visible, and the galaxy appears relatively undisturbed.
