The galaxy appears as an elliptical or lenticular type, showing a primarily smooth light distribution with a bright central bulge or core, and has an approximate diameter of 3.3 kpc. There is no evidence of spiral arm structure or significant dust lanes. The galaxy's shape is in between that of a circle and a cigar, implying it is moderately flattened. A subtle bluing is seen towards the center, and a redder hue around the outskirts suggesting a potential gradient in stellar populations, with younger stars being somewhat concentrated toward the center. There is no visual evidence of major mergers, tidal tails, or strong disturbances in its morphology, although minor interactions cannot be fully ruled out. Overall, the galaxy presents a relatively quiescent appearance.
