The galaxy presents a predominantly smooth morphology, suggesting an elliptical or lenticular classification. The light distribution is generally spheroidal, with a high degree of roundness. A small fraction of light is concentrated in a central bulge. There is no distinct disk component visible. The galaxy exhibits a red color, indicative of an older stellar population with suppressed star formation. Some minor disturbances can be observed, with a large population of nearby galaxies, indicating ongoing or past interactions. A significant percentage of light is indicative of a recent or ongoing merger.
