The galaxy presents a largely smooth morphology, appearing elliptical in shape with a high degree of roundness. There is little evidence of spiral arm structure or a defined disk. The central bulge is prominent, exhibiting a yellowish-orange hue, suggesting an older stellar population. A gradual decrease in color saturation and intensity is observed as one moves outwards from the core, with the outer regions displaying a more subdued blue-green tint. There appear to be no significant tidal tails, signs of recent mergers, or dust lanes visible. The galaxy's overall appearance indicates a relatively evolved system, likely with a low star formation rate. There is only a small chance that the galaxy is undergoing any merging.
