This galaxy presents a generally smooth appearance, suggesting an elliptical morphology or a spiral galaxy viewed at a high inclination. The central bulge is prominent and appears to be composed of older stellar populations, indicated by its yellowish-orange color. A faint disk may be present surrounding the bulge, but any spiral arm structure is not readily apparent. There appears to be some minor asymmetry in the light distribution, hinting at a possible past interaction or minor disturbance. A small, diffuse region of bluer light is located on one side of the galaxy, which might indicate an area of more recent star formation. The overall shape appears somewhat elongated, but not highly so. It appears as though a recent merger might be underway due to slight tidal tail formations.