The galaxy appears to be a relatively smooth, elliptical galaxy with a generally round morphology. There is little evidence of spiral arms or significant disk-like structure. The galaxy is concentrated towards the center, with a gradual decrease in luminosity outwards from the core. There is a slight elongation in its overall shape, but it is mostly spheroidal. It appears to be a fairly isolated galaxy with no signs of major mergers or strong tidal disturbances, with only a minor disturbance observed. The galaxy exhibits a relatively red color, indicating an older stellar population with less ongoing star formation, supported by the measured mass and star formation rate.
