The galaxy presents a generally smooth morphology, suggesting an elliptical or lenticular classification. It appears to be moderately luminous. Its shape is somewhat elongated rather than perfectly spherical. No obvious spiral arms or bar structures are discernible. There is a suggestion of a close companion galaxy. There is an indication of ongoing, although not dramatic, star formation activity. The galaxy shows a redder hue than expected, suggesting an older stellar population. Evidence for merging or major disturbance is minimal, although a minor disturbance could be present given the companion galaxy.
