This galaxy exhibits a morphology that is largely smooth and elliptical in nature. A concentrated central bulge dominates the structure with a yellowish hue, suggesting an older stellar population. Fainter, bluer regions are observed along the edges, hinting at more recent, though likely diminished, star formation activity. The galaxy appears to be relatively isolated, with no obvious signs of a major ongoing merger, although there is a slight asymmetry that might be interpreted as a minor tidal disturbance. The galaxy displays an intermediate apparent roundness, leaning more towards an elliptical shape than a perfectly circular one. 
