The galaxy presents a generally smooth, though not perfectly uniform, appearance. There's a suggestion of a disk-like structure, though the dominant impression is of a somewhat elongated spheroid. The light distribution within the galaxy suggests a higher concentration toward the central region. There may be minor disturbances visible, as the disk has a ragged edge. The overall color is intermediate, appearing neither distinctly blue (indicating active star formation) nor strongly red (suggesting an older stellar population). The estimated size is a few kiloparsecs across. The galaxy is likely of intermediate mass. There is evidence of it potentially being a merging galaxy. The overall star formation rate is low.
