The galaxy presents as an elliptical shape with a relatively smooth overall appearance, though it is exhibiting some internal structure. The central region presents a bright, condensed core that may indicate a high concentration of stars or possibly an active galactic nucleus. The galaxy displays a color gradient, transitioning from a more bluish hue in the outer regions to a yellow and white tone closer to the core. The bluer color in the periphery may suggest the presence of younger, hotter stars. There is a subtle hint of a disk, which could signify it being an edge-on spiral galaxy. Finally, there are small indications of minor disturbances in the galaxy's shape, possibly due to a past minor merger event.
