The galaxy presents a generally smooth, elliptical morphology. Its color profile is somewhat blueish, suggesting some level of ongoing star formation within the galaxy, although the primary stellar population seems to be more evolved, giving the galaxy an overall yellowish hue. The shape is more elongated, appearing somewhat cigar-shaped rather than perfectly circular, but the axial ratio doesn't suggest an edge-on disk galaxy. There are no obvious signs of major disturbances like tidal tails or significant asymmetry, indicating that major mergers may not have occurred recently. However, minor disturbances can't be ruled out, which may hint at past interactions with smaller satellite galaxies. The central region of the galaxy appears brighter and more concentrated, indicating a higher density of stars, potentially including a supermassive black hole at its nucleus.
