The galaxy presents a generally smooth, elliptical morphology. There is a slight elongation, appearing more cigar-shaped than perfectly round. A central bulge dominates the visual structure, emitting strongly in yellow light. The surrounding disk appears weakly visible, displaying a subtle blueish-green color gradient. No significant spiral arm structures or strong dust lanes are readily apparent. Overall, the galaxy's light is centrally concentrated, with a gradual decrease in intensity towards the outer regions. The lack of distinct features suggests minimal ongoing mergers or major disturbances, with a high probability of not merging at all.
