The galaxy appears as a diffuse, elliptical-shaped object. Its light distribution is relatively smooth, with a concentrated core region and a gradual fade towards the edges. The central region exhibits a brighter, more intense luminosity. The color profile is dominated by bluish hues, suggesting the presence of relatively young, hot stars or active star formation regions. There are some subtle irregularities or faint extensions visible, possibly indicative of tidal interactions or recent minor mergers. The overall structure leans towards an intermediate shape, neither perfectly spherical nor excessively elongated. Some evidence exists of minor disturbances in the morphology, but it appears to be largely unperturbed.
