This galaxy presents as a somewhat elliptical, disk-like structure. A central bulge is visible, appearing bright and concentrated, suggesting a high density of older stellar populations. The disk component exhibits a relatively smooth texture, but it also displays certain signs of disturbance. The disk does not appear to be in complete equilibrium. There are subtle asymmetrical features present, such as distortions or faint tidal tails or plumes, hinting at a possible interaction with another galaxy in the past or present. The color is generally yellow-red, consistent with light emitted from older stars. Areas of blue are also visible which may suggest there is current star formation present, although at a relatively low rate. The light intensity falls gradually from the center outwards and indicates a smooth transition between the bulge and the disk.
