The galaxy presents a primarily smooth morphology, showing a large central bulge with only a hint of a disk component. It exhibits an elliptical appearance, appearing more "in between" elliptical and circular than distinctly round or cigar-shaped. There are some minor disturbances, but overall, the galaxy appears relatively undisturbed, showing no signs of a major merger in its recent past. The galaxy appears to be a single object and not an obvious amalgamation of two or more galaxies.

The color profile shows a fairly even distribution of red, green, and blue light, indicating the presence of stars across a range of ages. The redder hues suggest a notable population of older, cooler stars. There is no evidence of high levels of on-going star formation. The galaxy is moderately luminous, suggesting that it is a massive galaxy.
