The galaxy appears to be an elliptical type, exhibiting a generally smooth and rounded morphology. There is a bright central bulge that gradually fades into the outer regions of the galaxy. The light distribution suggests a high degree of spherical symmetry. No distinct spiral arms or bar structures are visible. The color of the galaxy appears slightly reddish-yellow, possibly indicating an older stellar population and lower ongoing star formation rate. There might be some minor disturbances indicating the presence of some interactions. The galaxy does not appear to be undergoing a major merger or significant tidal disruption.
