The galaxy presents a generally smooth and rounded morphology. There is a high degree of central concentration, with a bright core that fades gradually into the outer regions. The galaxy appears elliptical in shape, with no discernible spiral arm structures. The overall color profile is consistent with an older stellar population. There are no signs of significant dust lanes, active star formation regions, or tidal disturbances, suggesting a quiescent state, with no ongoing or recent major merger events.
