The galaxy appears as an elliptical or lenticular type, with a smooth, diffuse light distribution and no discernible spiral arm structure. The color profile suggests a dominant older stellar population, exhibiting a yellowish-red hue. The galaxy's shape is roughly in between round and elongated. There is a possible minor disturbance in the galaxy's structure, which could indicate a small interaction or internal activity, although it is subtle. Overall, the galaxy appears to be relatively massive, with a moderate rate of star formation, and is at an estimated redshift of 0.23.
