The galaxy appears as a relatively smooth, elliptical-like structure. There is a concentrated central bulge that exhibits a yellowish hue, suggesting an older stellar population. The overall shape is not perfectly round but instead moderately elongated. There is a slight indication of a disturbance or faint tidal feature extending from the main body of the galaxy, however it is unclear if this is an indication of a possible merger. The outer regions of the galaxy show a radial decrease in luminosity. The galaxy is moderately bright in this image. The overall structure does not reveal distinct spiral arms or a well-defined disk component.
