The galaxy presents as a somewhat smooth, amorphous structure with a central concentration of light. The morphology appears predominantly elliptical, with a shape that is tending towards roundness. There is a hint of some irregularity in the distribution of light, with possible signs of a minor disturbance, and potentially a past merger event. The galaxy exhibits a reddish hue, suggesting an older stellar population. The galaxy is of substantial size, likely containing a significant stellar mass and is relatively faint, suggestive of being at a considerable distance. From visual inspection, it appears to be largely quiescent, with a correspondingly low rate of star formation.
