The galaxy appears to be an interacting system. The primary component is a large, relatively smooth galaxy, roughly elliptical in shape, with a concentrated central bulge. The color distribution suggests an older stellar population, with a dominant yellow-orange hue. There is evidence of possible tidal features extending from the main body, potentially indicating gravitational interaction.

A secondary component, smaller and more compact, is situated adjacent to the primary galaxy. This smaller galaxy exhibits a distinct reddish color. The system displays evidence of possible gravitational disturbance. There may be star formation occurring within both galaxies, but the primary galaxy appears to have a lower star formation rate compared to the smaller one.
