The galaxy presents a relatively smooth, elliptical morphology. It appears largely spheroidal with no prominent disk-like structure. There may be a minor interaction with another galaxy, or it could be showing some internal disturbance due to some past merging event. The galaxy displays a color gradient, transitioning from a more yellow/orange hue in its central region to somewhat redder tones in the outer parts. This color suggests an older stellar population. Judging by the distribution of light, the galaxy is likely a high-mass system. There doesn't appear to be significant ongoing star formation within the galaxy. The galaxy is measured to be roughly 12 kiloparsecs in radius.
