The galaxy presents a smooth, elliptical appearance with a slight elongation. It is dominated by a bright central bulge, which appears yellow-white in color, suggesting an older stellar population. A fainter, bluer region is visible, possibly indicating more recent star formation. The overall structure exhibits signs of gravitational disturbance or a potential merger event. A distinct tidal tail can be seen emanating from the main body, supporting the hypothesis of an ongoing interaction. The galaxy's morphology leans towards a merging system, hinting at a possible ongoing or recent collision with another galaxy.
