The galaxy presents an overall elliptical morphology, though not perfectly circular. There is a notable concentration of luminosity toward the central region. The light distribution appears relatively smooth, lacking distinct spiral arm structures or prominent dust lanes. The color gradient suggests the presence of an older stellar population, as evidenced by the relatively redder hue, particularly noticeable in the central bulge region. There is a hint of bluer light in the outer regions, indicating the presence of younger stars or active star formation, however this is a small effect. There is also an indication of a minor tidal disturbance.
