The galaxy presents a predominantly smooth morphology, appearing largely featureless without prominent spiral arms or a defined disk structure. Its shape is predominantly circular, exhibiting a high degree of roundness. There is no readily apparent evidence of significant ongoing or recent merger activity. The galaxy exhibits a concentrated central brightness, suggesting a well-defined galactic nucleus. The galaxy's color appears to be shifted towards the green part of the spectrum in this image. This could indicate younger, hotter stars or particular gas emissions, but the limited color information makes definitive statements on stellar populations difficult. Overall, this galaxy appears to be an elliptical galaxy with a smooth structure.
