This galaxy presents as an elliptical system, likely a relatively smooth and rounded structure when observed at higher resolutions. There is a slight cigar shape to its general form. The light distribution suggests a concentrated central bulge which fades gradually into a more diffuse halo. The core of the galaxy appears relatively bright, indicating a potentially significant concentration of stars and possibly a supermassive black hole at the center. While there is no obvious disk structure visible in this image, a slight blue-ish hue is present throughout the galaxy which could represent a small amount of star formation. Based on the absence of clear tidal features or major distortions, it appears relatively isolated and undisturbed. The presence of minor disturbances can not be ruled out from this image.
