The galaxy presents as a relatively smooth, elliptical structure. A central bulge is visible, exhibiting a yellowish hue, which may indicate an older stellar population. The outer regions show a decrease in surface brightness, with a hint of bluer tones in some areas, potentially indicative of younger stars or ongoing star formation in those regions. Overall, the galaxy does not exhibit any strong spiral arm structures or signs of major disturbances from mergers, but some minor disturbances cannot be ruled out. The shape appears to be somewhere between round and oblong.
