The galaxy presents as a largely featureless, elliptical morphology. The light distribution appears smooth and concentrated towards the center, with a high degree of circularity. The color profile is consistent with an older stellar population, exhibiting a yellow-orange hue that likely indicates a dominance of evolved stars. There is no discernible spiral arm structure or active star formation regions visible in this image. There is no indication of a strong tidal interaction or major merger events occurring in the recent past, although very faint signs of minor disturbances may be present. The galaxy appears to be relatively isolated.
