The galaxy presents a predominantly smooth morphology, exhibiting characteristics of an elliptical galaxy, though not perfectly spherical. The object displays an elongated shape, suggestive of a cigar-shaped structure. Color gradients indicate a central bulge region with an older stellar population, with an orange hue, which possibly indicates dust obscuration. There are very minor indications of a disk galaxy. Overall, the galaxy appears relatively undisturbed, with no major indications of ongoing or recent merger activity.
