The galaxy appears to be a relatively smooth, elliptical-like structure with a discernible elongated shape. The color profile leans toward the redder end of the spectrum, with a bright central bulge that diffuses outward. There are faint signs of possible tidal disturbances or interactions with a nearby companion galaxy, visible as a minor extension or bridge of light towards the smaller, rounder, neighboring structure. The general morphology indicates an evolved system with a low star formation rate. The smoothness suggests a lack of significant dust lanes or spiral arm structures. There might be an ongoing or past merger event contributing to the slightly distorted shape.
