The galaxy appears to be a luminous elliptical, exhibiting a smooth, diffuse light profile indicative of an older stellar population. The central region is bright yellow, suggesting a concentration of evolved stars. The overall morphology is largely spheroidal, with a high degree of roundness and a lack of discernible spiral arms or a prominent disk structure. There is a small object to the left of the main galaxy. A small disturbance is visible in the core of the galaxy, perhaps hinting towards a past merger event. The color index indicates a redder spectrum. The color suggests an older stellar population with ongoing, but low level, star formation. The estimated size of the galaxy indicates that it is a relatively large galaxy.
