The galaxy presents as a single, somewhat amorphous central structure with a smooth overall appearance. The light distribution is concentrated towards the center, suggestive of a high degree of central mass concentration. There are multiple distinct bright central components or knots visible within the galaxy's core, implying a possible ongoing or recent merger event. These knots exhibit different color properties, potentially indicating variations in stellar populations or levels of dust obscuration. The relatively smooth profile suggests a dominant spheroidal component. A faint, disturbed plume emanating from one of the knots supports the possibility of a recent interaction or merger, though without more data, it could simply be gas being ejected by high energy radiation. It appears relatively distant, as evidenced by its small apparent size and faintness. Overall, this appears to be a massive galaxy, likely elliptical or lenticular, with signs of past or ongoing interaction or merger activity.
