The galaxy appears as a relatively smooth, elliptical-like structure with a concentrated central bulge. It exhibits a yellowish hue in the central region, possibly indicating an older stellar population. The outer regions of the galaxy appear slightly bluer, suggesting the presence of some younger stars or ongoing star formation, though at a low rate. There is a hint of a flattened disk-like structure, but it is not strongly pronounced. Overall, it appears to be a fairly undisturbed system, with no obvious signs of major mergers or tidal distortions. The galaxy has a moderately compact size, and it is reasonably well-defined.
