The galaxy presents an elliptical morphology, appearing somewhat smooth with a high degree of roundness. There is a discernible central bulge, which is brighter and more concentrated than the outer regions of the galaxy. There is no strong evidence of spiral arm structure or a prominent disk component, though there is a very faint hint of a disk. There appears to be minimal star formation activity within the galaxy, as evidenced by the lack of bright blue regions often associated with star-forming regions. The galaxy is primarily yellowish-red in color, suggesting an older stellar population. Some minor gravitational disturbance cannot be ruled out, but overall, the galaxy appears relatively undisturbed.
