The galaxy appears to be an elliptical galaxy at a considerable distance. Its morphology is generally smooth and rounded, with the luminosity profile concentrated towards the center. There is a slight elongation, but overall it appears largely spheroidal.

The galaxy exhibits a color gradient, with a central yellowish-red hue that suggests an older stellar population and dust obscuration within the core. The outer regions display a slightly bluer tinge, possibly indicating more recent star formation at the periphery or a younger stellar population there. The overall color suggests that the galaxy is relatively passive, with a low rate of star formation. Some minor disturbances can be detected, but the overall shape looks relaxed with no signs of significant interaction with other galaxies, although a possible merger event in the past cannot be ruled out. There are indications of a faint, diffuse halo surrounding the main body of the galaxy, but it is not clearly defined.
