The galaxy presents as a generally smooth and rounded object. Its core exhibits a concentrated, bright yellowish-orange hue, suggesting an older stellar population or significant dust obscuration within the central region. The galaxy appears to lack prominent spiral arms or a well-defined disk structure. Fainter, greenish-blue emissions are observed in the outer regions, possibly indicating areas of more recent, albeit modest, star formation activity. There's no obvious evidence of any major ongoing mergers or significant tidal disturbances in this image. The overall morphology seems to be that of an elliptical galaxy, showing only very minor asymmetrical features.
