The galaxy presents an overall elliptical morphology, with a smooth and somewhat diffuse appearance. It exhibits a moderate elongation, appearing cigar-shaped. The color profile suggests an older stellar population, trending towards redder wavelengths, which is consistent with a passively evolving system. There is no apparent evidence of recent or ongoing star formation. No prominent spiral arm structures or dust lanes are discernible in the image, further supporting the classification as an elliptical galaxy with a likely substantial stellar mass. The galaxy appears relatively undisturbed, without any clear signs of major mergers or tidal interactions.
