The galaxy appears as a centrally concentrated object exhibiting a yellowish-white hue. Its morphology suggests a system undergoing some form of disturbance or interaction, exhibiting a non-smooth and somewhat irregular structure. There is a slight suggestion of a possible disk-like component, but it's heavily disrupted. The light profile is concentrated towards the center with a gradual decrease in intensity outward, spanning an estimated diameter of approximately 18 kpc. There is a possibility that this galaxy is merging with another object. This galaxy has intermediate mass. Star formation rate is very low for this galaxy.
