The galaxy appears as a moderately luminous, elongated object with a reddish-yellow hue. Its morphology suggests it is likely an elliptical galaxy, or possibly a spiral galaxy viewed edge-on. The light distribution shows a central concentration, with the intensity gradually decreasing outwards. There are some slight asymmetries in the outer regions, suggesting it could have experienced minor gravitational disturbances or a minor merger event in the past. There is no strong evidence of active star formation, based on the color distribution. The estimated size is a few kiloparsecs in radius.