The galaxy appears as a relatively smooth, elliptical-like object with a noticeable central bulge that is slightly elongated along a particular axis. There are subtle color gradients, with a slightly redder hue concentrated in the core region, suggesting an older stellar population. The outer regions exhibit a bluer tint indicating a younger, more active population of stars. The overall structure lacks defined spiral arms or prominent dust lanes. There is a faint indication of possible tidal features or minor disturbances, but that could also be noise in the data. The concentration of light is highest in the center, fading gradually outwards, characteristic of an early-type galaxy. The inferred stellar mass of the galaxy is substantial, with moderate levels of star formation activity.
