The galaxy presents a predominantly smooth morphology. The light is centrally concentrated, suggesting the presence of a bulge. Overall shape appears more in between round and elongated. There may be a faint hint of a disk-like structure but it is not well-defined. The object shows no signs of major merging activity, although a minor disturbance or possible companion cannot be ruled out due to the slightly irregular outskirts. The galaxy exhibits an apparent red shift. Based on its estimated size, its luminosity indicates it falls roughly within the range of a fairly bright galaxy. Star formation rate is on the lower end, placing it amongst galaxies undergoing less active star formation. The stellar mass appears to be on the higher side.
