The galaxy appears as a relatively smooth, elliptical-like structure with a concentrated central bulge. The color profile indicates a bias towards older stellar populations, as evidenced by its yellow-red hue. There is a slight deviation from perfect circularity, showing a subtle elongation. There is little indication of active star formation regions, instead appearing mostly quiescent. It appears isolated, exhibiting no strong tidal interactions or signs of ongoing mergers with other significant galaxies nearby. A very small hint of bluer light is seen in some small patches, but the overall galaxy has a smooth appearance with no spiral arm-like features.
